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<title>Prokyon</title>

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<h1 id="firstHeading" class="firstHeading mw-first-heading">Prokyon</h1>

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</style><div id="coordinates" class="coordinates"><a class="external text" href="https://geohack.toolforge.org/skyhack.php?ra=7.6550277777778&de=5.225&size=0.033333333333333&name=Prokyon+%28%CE%B1+Canis+Minoris%29&object=Alpha%20CMi&_globe:=">Datenbanklinks zu Prokyon (α Canis Minoris)</a></div>

<th colspan="3" class="ibheader">Doppelstern Prokyon (α Canis Minoris)

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<td colspan="3" class="ibimgtxt notheme">Prokyon ist der hellste Stern im Sternbild Canis Minor (unten links)

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<td colspan="3" class="ibmap notheme"><div style="position:relative;"><table style="border:0; width:310px; text-align:left; display:inline-table;"><tbody><tr><td style="border:0; padding:0;"><div style="position: relative;"><div style="position: absolute; display: block; padding:0px; margin:0px; left:137.15434891905px; top:241.57868275515px;"></div></div></td></tr></tbody></table>Vorlage:Skymap/Wartung/CMi</div>

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<td colspan="3" class="ibmaptxt notheme">Lage des Sterns im Sternbild Kleiner Hund

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<th colspan="3" class="ibheader">Beobachtungsdaten <a href="%C3%84quinoktium" title="Äquinoktium">Äquinoktium</a>: <a href="Epoche_(Astronomie)#Standardepochen" title="Epoche (Astronomie)">J2000.0</a>, <a href="Epoche_(Astronomie)" title="Epoche (Astronomie)">Epoche</a>: J2000.0

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<td colspan="3" style="text-align:center;"><a rel="nofollow" class="external text" href="https://aladin.cds.unistra.fr/AladinLite/?target=07%2039%2018.1%20%2B05%2013%2030.0&fov=0.033333333333333&survey=CDS%2FP%2FDSS2%2Fcolor">AladinLite</a>

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<td><a href="Sternbild" title="Sternbild">Sternbild</a>

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<td colspan="2" class="ibnowrap"><a href="Kleiner_Hund" title="Kleiner Hund">Kleiner Hund</a>

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<td><a href="Rektaszension" title="Rektaszension">Rektaszension</a>

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<td><a href="Deklination_(Astronomie)" title="Deklination (Astronomie)">Deklination</a>

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<td><a href="Scheinbare_Helligkeit" title="Scheinbare Helligkeit">Scheinbare Helligkeit</a> <a href="#cite_note-Simbad-1">[1]</a><a href="#cite_note-Simbad2-2">[2]</a>

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<td colspan="2" class="ibnowrap">0,37 mag

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<td>Bekannte <a href="Exoplanet" title="Exoplanet">Exoplaneten</a>

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{{{Planeten}}}

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<td colspan="3" class="ibheader">Position des Begleiters

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<td>Winkelabstand

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<td colspan="2" class="ibnowrap">{{{Winkelabstand}}}

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<td><a href="Positionswinkel" title="Positionswinkel">Positionswinkel</a>

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<td colspan="2" class="ibnowrap">{{{Positionswinkel}}}

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<th colspan="3" class="ibheader"><a href="Astrometrie" title="Astrometrie">Astrometrie</a>

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<td><a href="Radialgeschwindigkeit" title="Radialgeschwindigkeit">Radialgeschwindigkeit</a>

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<td><a href="Parallaxe" title="Parallaxe">Parallaxe</a>

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<td>Entfernung

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<td colspan="2" class="ibnowrap">(11,41 ± 0,04) <a href="Lichtjahr" title="Lichtjahr">Lj</a> ((3,497 ± 0,011) <a href="Parsec" title="Parsec">pc</a>)

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<td><a href="Absolute_Helligkeit" title="Absolute Helligkeit">Absolute visuelle Helligkeit</a> Mvis

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<td colspan="2" class="ibnowrap">mag

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<td><a href="Absolute_Helligkeit" title="Absolute Helligkeit">Absolute bolometrische Helligkeit</a> Mbol

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<td colspan="2" class="ibnowrap">mag

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<td colspan="3" style="color:#ff0000;text-align:center;">Veralteter Parameter "Absolut" !

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<th colspan="3" class="ibheader"><a href="Eigenbewegung_(Astronomie)" title="Eigenbewegung (Astronomie)">Eigenbewegung</a>

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<td>Rektaszensionsanteil:

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<td>Deklinationsanteil:

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<th colspan="3" class="ibheader">Orbit

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<td><a href="Umlaufzeit" title="Umlaufzeit">Periode</a>

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<td><a href="Halbachsen_der_Ellipse" title="Halbachsen der Ellipse">Große Halbachse</a>

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<td><a href="Exzentrizit%C3%A4t_(Astronomie)" title="Exzentrizität (Astronomie)">Exzentrizität</a>

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<td><a href="Apsis_(Astronomie)" title="Apsis (Astronomie)">Periastron</a>

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<td><a href="Apsis_(Astronomie)" title="Apsis (Astronomie)">Apastron</a>

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<td><a href="Bahnneigung" title="Bahnneigung">Bahnneigung</a>

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<td><a href="Argument_des_Knotens" class="mw-redirect" title="Argument des Knotens">Argument des Knotens</a>

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<td>Epoche des Periastrons

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<td>Argument der Periapsis

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<th colspan="3" class="ibheader">Einzeldaten

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<td>Namen

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<td colspan="2" style="white-space:nowrap;">A; B

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<td colspan="3" class="ibheadercomp">Beobachtungsdaten

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<td rowspan="2" style="vertical-align:middle"><a href="Scheinbare_Helligkeit" title="Scheinbare Helligkeit">Scheinbare Helligkeit</a> <a href="#cite_note-Simbad-1">[1]</a><a href="#cite_note-Simbad2-2">[2]</a>

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<td>A

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<td style="white-space:nowrap;">+0,37 mag

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<td>B

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<td style="white-space:nowrap;">10,92 mag

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<td colspan="3" class="ibheadercomp">Spektrum und Indices

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<td rowspan="2" style="vertical-align:middle"><a href="Spektralklasse" title="Spektralklasse">Spektralklasse</a><a href="#cite_note-Simbad-1">[1]</a>

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<td>A

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<td style="white-space:nowrap;">F5 IV-V

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<td>B

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<td style="white-space:nowrap;">DQZ

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<td rowspan="2" style="vertical-align:middle">B−V-<a href="Farbindex" title="Farbindex">Farbindex</a><a href="#cite_note-Simbad-1">[1]</a><a href="#cite_note-Simbad2-2">[2]</a>

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<td>A

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<td style="white-space:nowrap;">(+0,42)

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<td>B

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<td style="white-space:nowrap;">(−0,22)

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<td style="vertical-align:middle">U−B-Farbindex<a href="#cite_note-Simbad-1">[1]</a>

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<td>A

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<td style="white-space:nowrap;">(+0,03)

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<td colspan="3" class="ibheadercomp">Physikalische Eigenschaften

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<td rowspan="2" style="vertical-align:middle"><a href="Absolute_Helligkeit" title="Absolute Helligkeit">Absolute vis. Helligkeit</a> Mvis<a href="#cite_note-ApJ119_2-4">[4]</a>

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<td>A

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<td style="white-space:nowrap;">+2,7 mag

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<td>B

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<td style="white-space:nowrap;">+13 mag

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<td rowspan="2" style="vertical-align:middle"><a href="Masse_(Physik)" title="Masse (Physik)">Masse</a><a href="#cite_note-Liebert2013-5">[5]</a><a href="#cite_note-Provencal2002-6">[6]</a>

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<td>A

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<td>B

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<td rowspan="2" style="vertical-align:middle"><a href="Radius" title="Radius">Radius</a><a href="#cite_note-aaa413-7">[7]</a><a href="#cite_note-Provencal2002-6">[6]</a>

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<td>A

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<td>B

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<td rowspan="2" style="vertical-align:middle"><a href="Leuchtkraft" title="Leuchtkraft">Leuchtkraft</a><a href="#cite_note-aaa413-7">[7]</a><a href="#cite_note-ApJS199_2_29-8">[8]</a>

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<td>A

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<td>B

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<td rowspan="2" style="vertical-align:middle"><a href="Effektive_Temperatur" title="Effektive Temperatur">Effektive Temperatur</a><a href="#cite_note-aaa413-7">[7]</a><a href="#cite_note-Provencal2002-6">[6]</a>

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<td>A

</td>

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<td>B

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<td rowspan="2" style="vertical-align:middle"><a href="Rotation_(Physik)" title="Rotation (Physik)">Rotationsdauer</a>

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<td>A

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<td>B

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<td>Alter

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<td colspan="2" style="white-space:nowrap;">1,7 Mrd. Jahre

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<th colspan="3" class="ibheader">Andere Bezeichnungen und <a href="Liste_astronomischer_Kataloge" title="Liste astronomischer Kataloge">Katalogeinträge</a>

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<td colspan="3" style="padding:0;"><table class="wikitable" style="box-sizing:border-box; width:100%; font-size:smaller; margin:0; border-collapse:collapse;"><tbody><tr><th style="white-space:nowrap;">Katalog</th><th>A</th><th>B</th></tr><tr><td style="white-space:nowrap;"><a href="Bayer-Bezeichnung" title="Bayer-Bezeichnung">Bayer-Bezeichnung</a></td><td colspan="2" style="white-space:nowrap;">α Canis Minoris</td></tr><tr><td style="white-space:nowrap;"><a href="Flamsteed-Bezeichnung" title="Flamsteed-Bezeichnung">Flamsteed-Bezeichnung</a></td><td colspan="2" style="white-space:nowrap;">10 Canis Minoris</td></tr><tr><td style="white-space:nowrap;"><a href="Bonner_Durchmusterung" title="Bonner Durchmusterung">Bonner Durchmusterung</a></td><td colspan="2" style="white-space:nowrap;"> BD +5° 1739</td></tr><tr><td style="white-space:nowrap;"><a href="Sternkatalog#Gliese_(Gl)_und_Gliese-Jahreiß_(GJ)" title="Sternkatalog">Gliese-Katalog</a></td><td colspan="2" style="white-space:nowrap;"> GJ 280 <a rel="nofollow" class="external autonumber" href="https://vizier.u-strasbg.fr/viz-bin/VizieR-S?GJ%20280">[1]</a></td></tr><tr><td style="white-space:nowrap;"><a href="Bright-Star-Katalog" title="Bright-Star-Katalog">Bright-Star-Katalog</a></td><td colspan="2" style="white-space:nowrap;">HR 2943 <a rel="nofollow" class="external autonumber" href="https://cdsarc.u-strasbg.fr/viz-bin/VizieR-5?-source=V/50&-out.all&-out.max=10&HR==2943">[2]</a></td></tr><tr><td style="white-space:nowrap;"><a href="Henry-Draper-Katalog" title="Henry-Draper-Katalog">Henry-Draper-Katalog</a></td><td colspan="2" style="white-space:nowrap;">HD 61421 <a rel="nofollow" class="external autonumber" href="https://cdsarc.u-strasbg.fr/viz-bin/VizieR-5?-source=III/135A/catalog&-out.all&-out.max=10&HD==61421">[3]</a></td></tr><tr><td style="white-space:nowrap;"><a href="SAO-Katalog" title="SAO-Katalog">SAO-Katalog</a></td><td colspan="2" style="white-space:nowrap;">SAO 115756 <a rel="nofollow" class="external autonumber" href="https://cdsarc.u-strasbg.fr/viz-bin/VizieR-5?-source=I/131A/sao&-out.all&-out.max=10&SAO==115756">[4]</a></td></tr><tr><td style="white-space:nowrap;"><a href="Hipparcos-Katalog" title="Hipparcos-Katalog">Hipparcos-Katalog</a></td><td colspan="2" style="white-space:nowrap;">HIP 37279 <a rel="nofollow" class="external autonumber" href="https://vizier.u-strasbg.fr/viz-bin/VizieR-5?-source=I/311&-out.all&-out.max=10&HIP==37279">[5]</a></td></tr><tr><td style="white-space:nowrap;">Weitere Bezeichnungen:</td><td colspan="2">

Prokyon • LHS 233 • <a href="FK5" title="FK5">FK5</a> 291</td>

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Prokyon [proˈkyɔn] (α Canis Minoris; Synonyme: Elgomaisa, Algomeysa, Antecanis; <a href="Alt%C3%A4gyptische_Sprache" title="Altägyptische Sprache">altägyptisch</a> <a href="Imi-chet-Sopdet" title="Imi-chet-Sopdet">Imi-chet-Sopdet</a>; früher ebenso wie <a href="Sirius" title="Sirius">Sirius</a> auch Aschere oder Canicula genannt<a href="#cite_note-MathLex1734-9">[9]</a>) ist der hellste <a href="Stern" title="Stern">Stern</a> im <a href="Sternbild" title="Sternbild">Sternbild</a> <a href="Kleiner_Hund" title="Kleiner Hund">Kleiner Hund</a>. Mit einer Entfernung von 11,4 <a href="Lichtjahr" title="Lichtjahr">Lichtjahren</a> ist er einer der sonnennächsten Sterne. Der griechische Name bedeutet „vor dem Hund“ und weist darauf hin, dass er vor Sirius, dem Hundsstern aufgeht.

<div class="mw-heading mw-heading2"><h2 id="Beschreibung">Beschreibung</h2></div>

Prokyon ist Bestandteil des <a href="Wintersechseck" title="Wintersechseck">Wintersechsecks</a> und des <a href="Winterdreieck" title="Winterdreieck">Winterdreiecks</a>. Wie Sirius ist Prokyon ein <a href="Doppelstern" title="Doppelstern">Doppelstern</a> – der Hauptstern Prokyon A, ein weißlich-gelber Stern der <a href="Spektralklasse" title="Spektralklasse">Spektralklasse</a> F5, hat einen leuchtschwachen Begleiter 11. Größe, Prokyon B, der ein <a href="Wei%C3%9Fer_Zwerg" title="Weißer Zwerg">Weißer Zwerg</a> ist. Die Umlaufperiode des Doppelsternsystems beträgt 41 Jahre. Der scheinbare Winkelabstand beträgt ca. 4,7″.<a href="#cite_note-ApJ119_2-4">[4]</a>

<div class="mw-heading mw-heading2"><h2 id="Sonstiges">Sonstiges</h2></div>

Prokyon ist in der <a href="Flagge_Brasiliens" title="Flagge Brasiliens">Flagge Brasiliens</a> abgebildet, wo er den Bundesstaat <a href="Amazonas_(Brasilien)" title="Amazonas (Brasilien)">Amazonas</a> repräsentiert.

<div class="mw-heading mw-heading2"><h2 id="Weblinks">Weblinks</h2></div>

<div class="sisterproject" style="margin:0.1em 0 0 0;"><div class="noresize noviewer" style="display:inline-block; line-height:10px; min-width:1.6em; text-align:center;" aria-hidden="true" role="presentation"></div><a class="external text" href="https://commons.wikimedia.org/wiki/Category:Procyon_(star)?uselang=de">Commons: Prokyon</a> – Sammlung von Bildern, Videos und Audiodateien</div>

<ul><li><a rel="nofollow" class="external free" href="http://stars.astro.illinois.edu/sow/procyon.html">http://stars.astro.illinois.edu/sow/procyon.html</a></li></ul>

<div class="mw-heading mw-heading2"><h2 id="Einzelnachweise">Einzelnachweise</h2></div>

<li id="cite_note-Simbad-1">↑ <a href="#cite_ref-Simbad_1-0">a</a> <a href="#cite_ref-Simbad_1-1">b</a> <a href="#cite_ref-Simbad_1-2">c</a> <a href="#cite_ref-Simbad_1-3">d</a> <a href="#cite_ref-Simbad_1-4">e</a> <a href="#cite_ref-Simbad_1-5">f</a> <a rel="nofollow" class="external text" href="http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=procyon&submit=SIMBAD+search">alf CMi.</a> In: <a href="SIMBAD" title="SIMBAD">SIMBAD</a>. <a href="Centre_de_Donn%C3%A9es_astronomiques_de_Strasbourg" title="Centre de Données astronomiques de Strasbourg">Centre de Données astronomiques de Strasbourg</a>, abgerufen am 18. September 2018.<span style="display: none;" class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2Fde.wikipedia.org%3AProkyon&rft.title=alf+CMi&rft.description=alf+CMi&rft.identifier=http%3A%2F%2Fsimbad.u-strasbg.fr%2Fsimbad%2Fsim-basic%3FIdent%3Dprocyon%26submit%3DSIMBAD%2Bsearch&rft.publisher=%5B%5BCentre+de+Donn%C3%A9es+astronomiques+de+Strasbourg%5D%5D">

</li>

<li id="cite_note-Simbad2-2">↑ <a href="#cite_ref-Simbad2_2-0">a</a> <a href="#cite_ref-Simbad2_2-1">b</a> <a rel="nofollow" class="external text" href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=@988144&Name=*%20alf%20CMi%20B&submit=submit">alf CMi B.</a> In: SIMBAD. Centre de Données astronomiques de Strasbourg, abgerufen am 18. September 2018.<span style="display: none;" class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2Fde.wikipedia.org%3AProkyon&rft.title=alf+CMi+B&rft.description=alf+CMi+B&rft.identifier=http%3A%2F%2Fsimbad.u-strasbg.fr%2Fsimbad%2Fsim-id%3FIdent%3D%2540988144%26Name%3D%2A%2520alf%2520CMi%2520B%26submit%3Dsubmit&rft.publisher=Centre+de+Donn%C3%A9es+astronomiques+de+Strasbourg">

</li>

<li id="cite_note-Hip1-3"><a href="#cite_ref-Hip1_3-0">↑</a> <a rel="nofollow" class="external text" href="http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%20%2037279">Hipparcos-Katalog (1997)</a>

</li>

<li id="cite_note-ApJ119_2-4">↑ <a href="#cite_ref-ApJ119_2_4-0">a</a> <a href="#cite_ref-ApJ119_2_4-1">b</a> Daniel J. Schroeder, David A. Golimowski, Ryan A. Brukardt, Christopher J. Burrows, John J. Caldwell, William G. Fastie, Holland C. Ford, Brigette Hesman, Ilona Kletskin, John E. Krist, Patricia Royle, Richard. A. Zubrowski: <cite style="font-style:italic">A Search for Faint Companions to Nearby Stars Using the Wide Field Planetary Camera 2</cite>. In: <cite style="font-style:italic"><a href="The_Astronomical_Journal" class="mw-redirect" title="The Astronomical Journal">The Astronomical Journal</a></cite>. 119. Jahrgang, Nr. 2, Februar 2000, S. 906–922, <a href="Digital_Object_Identifier" title="Digital Object Identifier">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1086/301227">10.1086/301227</a>, <a href="Bibcode" title="Bibcode">bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2000AJ....119..906S">2000AJ....119..906S</a>.<span class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rfr_id=info:sid/de.wikipedia.org:Prokyon&rft.atitle=A+Search+for+Faint+Companions+to+Nearby+Stars+Using+the+Wide+Field+Planetary+Camera+2&rft.au=Daniel+J.%26%2332%3BSchroeder%2C%26%2332%3BDavid+A.%26%2332%3BGolimowski%2C%26%2332%3BRyan+A.%26%2332%3BBrukardt%2C+...&rft.date=2000-02&rft.doi=10.1086%2F301227&rft.genre=journal&rft.issue=2&rft.jtitle=The+Astronomical+Journal&rft.pages=906-922&rft.volume=119.+Jahrgang" style="display:none">

</li>

<li id="cite_note-Liebert2013-5"><a href="#cite_ref-Liebert2013_5-0">↑</a> James Liebert, Gilles Fontaine, Patrick A. Young, Kurtis A. Williams, David Arnett: <cite style="font-style:italic">The Age and Stellar Parameters of the Procyon Binary System</cite>. In: <cite style="font-style:italic"><a href="The_Astrophysical_Journal" title="The Astrophysical Journal">The Astrophysical Journal</a></cite>. 769. Jahrgang, Nr. 1, Mai 2013, 7, S. 10, <a href="Digital_Object_Identifier" title="Digital Object Identifier">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1088/0004-637X%2F769%2F1%2F7">10.1088/0004-637X/769/1/7</a>, <a href="ArXiv" title="ArXiv">arxiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/1305.0587">1305.0587</a>, <a href="Bibcode" title="Bibcode">bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2013ApJ...769....7L">2013ApJ...769....7L</a>.<span class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rfr_id=info:sid/de.wikipedia.org:Prokyon&rft.atitle=The+Age+and+Stellar+Parameters+of+the+Procyon+Binary+System&rft.au=James%26%2332%3BLiebert%2C%26%2332%3BGilles%26%2332%3BFontaine%2C%26%2332%3BPatrick+A.%26%2332%3BYoung%2C+...&rft.date=2013-05&rft.doi=10.1088%2F0004-637X%2F769%2F1%2F7&rft.genre=journal&rft.issue=1&rft.jtitle=The+Astrophysical+Journal&rft.pages=10&rft.volume=769.+Jahrgang" style="display:none">

</li>

<li id="cite_note-Provencal2002-6">↑ <a href="#cite_ref-Provencal2002_6-0">a</a> <a href="#cite_ref-Provencal2002_6-1">b</a> <a href="#cite_ref-Provencal2002_6-2">c</a> J. L. Provencal, H. L. Shipman, Detlev Koester, F. Wesemael, P. Bergeron: <cite style="font-style:italic">Procyon B: Outside the Iron Box</cite>. In: <cite style="font-style:italic">The Astrophysical Journal</cite>. 568. Jahrgang, Nr. 1, 2002, S. 324–334, <a href="Digital_Object_Identifier" title="Digital Object Identifier">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1086/338769">10.1086/338769</a>, <a href="Bibcode" title="Bibcode">bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2002ApJ...568..324P">2002ApJ...568..324P</a>.<span class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rfr_id=info:sid/de.wikipedia.org:Prokyon&rft.atitle=Procyon+B%3A+Outside+the+Iron+Box&rft.au=J.+L.%26%2332%3BProvencal%2C%26%2332%3BH.+L.%26%2332%3BShipman%2C%26%2332%3BDetlev%26%2332%3BKoester%2C+...&rft.date=2002&rft.doi=10.1086%2F338769&rft.genre=journal&rft.issue=1&rft.jtitle=The+Astrophysical+Journal&rft.pages=324-334&rft.volume=568.+Jahrgang" style="display:none">

</li>

<li id="cite_note-aaa413-7">↑ <a href="#cite_ref-aaa413_7-0">a</a> <a href="#cite_ref-aaa413_7-1">b</a> <a href="#cite_ref-aaa413_7-2">c</a> P. Kervella, F. Thévenin, P. Morel, G. Berthomieu, P. Bordé, J. Provost: <cite style="font-style:italic">The diameter and evolutionary state of Procyon A. Multi-technique modeling using asteroseismic and interferometric constraints</cite>. In: <cite style="font-style:italic"><a href="Astronomy_and_Astrophysics" class="mw-redirect" title="Astronomy and Astrophysics">Astronomy and Astrophysics</a></cite>. 413. Jahrgang, Nr. 1, Januar 2004, S. 251–256, <a href="Digital_Object_Identifier" title="Digital Object Identifier">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1051/0004-6361%3A20031527">10.1051/0004-6361:20031527</a>, <a href="ArXiv" title="ArXiv">arxiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/astro-ph/0309148">astro-ph/0309148</a>, <a href="Bibcode" title="Bibcode">bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2004A&A...413..251K">2004A&A...413..251K</a>.<span class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rfr_id=info:sid/de.wikipedia.org:Prokyon&rft.atitle=The+diameter+and+evolutionary+state+of+Procyon+A.+Multi-technique+modeling+using+asteroseismic+and+interferometric+constraints&rft.au=P.%26%2332%3BKervella%2C%26%2332%3BF.%26%2332%3BTh%C3%A9venin%2C%26%2332%3BP.%26%2332%3BMorel%2C+...&rft.date=2004-01&rft.doi=10.1051%2F0004-6361%3A20031527&rft.genre=journal&rft.issue=1&rft.jtitle=Astronomy+and+Astrophysics&rft.pages=251-256&rft.volume=413.+Jahrgang" style="display:none">

</li>

<li id="cite_note-ApJS199_2_29-8"><a href="#cite_ref-ApJS199_2_29_8-0">↑</a> N. Giammichele, P. Bergeron, P. Dufour: <cite style="font-style:italic">Know Your Neighborhood: A Detailed Model Atmosphere Analysis of Nearby White Dwarfs</cite>. In: <cite style="font-style:italic">The Astrophysical Journal Supplement</cite>. 199. Jahrgang, Nr. 2, April 2012, S. 29, <a href="Digital_Object_Identifier" title="Digital Object Identifier">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1088/0067-0049%2F199%2F2%2F29">10.1088/0067-0049/199/2/29</a>, <a href="ArXiv" title="ArXiv">arxiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/1202.5581">1202.5581</a>, <a href="Bibcode" title="Bibcode">bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2012ApJS..199...29G">2012ApJS..199...29G</a>.<span class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rfr_id=info:sid/de.wikipedia.org:Prokyon&rft.atitle=Know+Your+Neighborhood%3A+A+Detailed+Model+Atmosphere+Analysis+of+Nearby+White+Dwarfs&rft.au=N.%26%2332%3BGiammichele%2C%26%2332%3BP.%26%2332%3BBergeron%2C%26%2332%3BP.%26%2332%3BDufour&rft.date=2012-04&rft.doi=10.1088%2F0067-0049%2F199%2F2%2F29&rft.genre=journal&rft.issue=2&rft.jtitle=The+Astrophysical+Journal+Supplement&rft.pages=29&rft.volume=199.+Jahrgang" style="display:none">  Age is for the white dwarf stage.

</li>

<li id="cite_note-MathLex1734-9"><a href="#cite_ref-MathLex1734_9-0">↑</a> <a href="Christian_Wolff_(Aufkl%C3%A4rer)" title="Christian Wolff (Aufklärer)">Christian Wolff</a>: <a rel="nofollow" class="external text" href="https://books.google.ch/books?id=KpgvdmGpIZQC&pg=PA645&dq=Aschere,+Canicula">Hund.</a> In: Vollständiges Mathematisches Lexicon. <a href="Johann_Friedrich_Gleditsch" title="Johann Friedrich Gleditsch">Johann Friedrich Gleditschens</a> seel. Sohn, 1734, abgerufen am 8. Juni 2021.<span style="display: none;" class="Z3988" title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2Fde.wikipedia.org%3AProkyon&rft.title=Hund&rft.description=Hund&rft.identifier=https%3A%2F%2Fbooks.google.ch%2Fbooks%3Fid%3DKpgvdmGpIZQC%26pg%3DPA645%26dq%3DAschere%2C%2BCanicula&rft.creator=%5B%5BChristian+Wolff+%28Aufkl%C3%A4rer%29%7CChristian+Wolff%5D%5D&rft.publisher=%5B%5BJohann+Friedrich+Gleditsch%5D%5Dens+seel.+Sohn&rft.date=1734">

</li>

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