Estrela (astronomía): Diferenzas entre revisións
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Liña 41:
Normalmente as estrelas inician a súa combustión nuclear cun 75% de [[hidróxeno]] e un 25% de [[helio]] xunto con pequenas trazas de outros elementos.
==Véxase tamén==
{{commonscat|Star}}
===Bibliografía===
* {{cite book | first1=Cliff | last1=Pickover | authorlink = Cliff Pickover | year=2001 |title=The Stars of Heaven | publisher=Oxford University Press | isbn=0-19-514874-6}}
* {{cite book | first1=John | last1=Gribbin | authorlink = John Gribbin | first2=Mary | last2=Gribbin | year=2001 | title=Stardust: Supernovae and Life—The Cosmic Connection | publisher=[[Yale University Press]] | isbn=0-300-09097-8}}
* {{cite book | first1=Stephen | last2=Hawking | title=A Brief History of Time | authorlink=Stephen Hawking | year=1988 | publisher=Bantam Books | isbn=0-553-17521-1}}
===Ligazóns externas===
* {{cite web | last=Kaler | first=James | title=Portraits of Stars and their Constellations | publisher=University of Illinois | url=http://stars.astro.illinois.edu/sow/sow.html}}
* {{cite web | title=Query star by identifier, coordinates or reference code | work=SIMBAD | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-fid}}
* {{cite web | title=How To Decipher Classification Codes | publisher=Astronomical Society of South Australia | url=http://www.assa.org.au/sig/variables/classifications.asp}}
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[[Categoría:Obxectos astronómicos]]
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