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Anomalous Cepheid variable stars original
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Cepheid variable stars original
Solar analogs original
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Stellar types original
History of astronomy original
star this property dcterms created equal to or less than 2018-09-17T19:35:00Zequal to or more than 2018-09-17T19:35:00Z
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Interdisciplinary astronomy original
Gamma Doradus variable stars original
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Pulsating variable stars original
CEMP stars original
star this property dcterms created equal to or less than 2018-09-17T18:11:30Zequal to or more than 2018-09-17T18:11:30Z
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Chemically peculiar stars original
B(e) stars original
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Be stars original
Field stars original
star this property dcterms created equal to or less than 2018-09-14T19:11:19Zequal to or more than 2018-09-14T19:11:19Z
unstar this property dcterms modified equal to or less than 2018-09-14T19:14:04Zequal to or more than 2018-09-14T19:14:04Z
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Stellar types original
star this property definition "A star that does not belong to a stellar cluster, but happens to be adjacent to it." - An Etymological Dictionary of Astronomy and Astrophysics, by M. Heydari-Malayeri.
Stellar granulation original
star this property dcterms created equal to or less than 2018-09-14T16:58:41Zequal to or more than 2018-09-14T16:58:41Z
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Stellar physics original
Asymptotic giant branch stars original
star this property dcterms created equal to or less than 2018-09-13T21:08:20Zequal to or more than 2018-09-13T21:08:20Z
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Stellar evolutionary types original
Stellar spectral types original
star this property dcterms created equal to or less than 2018-09-13T17:13:21Zequal to or more than 2018-09-13T17:13:21Z
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Stellar types original
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A stars original
B stars original
F stars original
G stars original
K stars original
M stars original
O stars original
OB stars original
R stars original
S stars original
Subdwarf stars original
star this property dcterms created equal to or less than 2018-09-13T17:00:21Zequal to or more than 2018-09-13T17:00:21Z
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Stellar evolutionary types original
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A subdwarf stars original
B subdwarf stars original
F subdwarf stars original
G subdwarf stars original
O subdwarf stars original
T subdwarfs original
Dwarf stars original
star this property dcterms created equal to or less than 2018-09-13T17:00:09Zequal to or more than 2018-09-13T17:00:09Z
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Stellar evolutionary types original
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A dwarf stars original
B dwarf stars original
F dwarf stars original
G dwarf stars original
K dwarf stars original
M dwarf stars original
O dwarf stars original
T dwarfs original
Stellar evolutionary types original
star this property dcterms created equal to or less than 2018-09-13T16:55:49Zequal to or more than 2018-09-13T16:55:49Z
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Stellar types original
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Dwarf stars original
Subdwarf stars original
Asymptotic giant branch stars original
Blue straggler stars original
Brown dwarfs original
Evolved stars original
Horizontal branch stars original
Main sequence stars original
Pre-main sequence stars original
White dwarf stars original
Yellow straggler stars original
Horizontal branch original
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Hertzsprung Russell diagram original
Main sequence original
star this property dcterms created equal to or less than 2018-09-13T14:54:24Zequal to or more than 2018-09-13T14:54:24Z
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Hertzsprung Russell diagram original
Stellar evolutionary models original
star this property dcterms created equal to or less than 2018-09-13T14:51:48Zequal to or more than 2018-09-13T14:51:48Z
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Astronomical research original
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Hertzsprung Russell diagram original
Stellar evolutionary tracks original
Schonberg-Chandrasekhar limit original
star this property dcterms created equal to or less than 2018-09-10T16:07:43Zequal to or more than 2018-09-10T16:07:43Z
unstar this property dcterms modified equal to or less than 2018-09-11T18:40:36Zequal to or more than 2018-09-11T18:40:36Z
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Gravitational collapse original
star this property definition This represents the maximum fraction of a star's mass that can be contained within an isothermal core while still supporting the rest of the star in hydrostatic equilibrium. Once the mass of an isothermal helium core exceeds this limit, the corse collapses and the star evolve rapidly. The limit varies depending on the star.
Stellar M coronal regions original
star this property dcterms created equal to or less than 2018-09-07T22:00:04Zequal to or more than 2018-09-07T22:00:04Z
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Stellar coronae original
Solar K coronal region original
star this property dcterms created equal to or less than 2018-09-07T21:44:38Zequal to or more than 2018-09-07T21:44:38Z
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Solar corona original
Cosmic background radiation original
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Recombination (cosmology) original
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Cosmic microwave background radiation original
Galactic bulge original
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Milky Way Galaxy physics original
Galaxy quenching original
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Galaxy evolution original
Solar coronal plumes original
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Solar corona original
Solar coronal lines original
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Solar corona original
X-ray active galactic nuclei original
star this property dcterms created equal to or less than 2018-09-06T14:42:59Zequal to or more than 2018-09-06T14:42:59Z
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Active galactic nuclei original