Subraksasa: Perbedaan antara revisi

Sub-Raksasa adalah bintang yang lebih terang daripada bintang deret utama normal pada kelas spektral yang sama, tetapi tidak seterang bintang raksasa. Istilah "Sub-Raksasa" diterapkan baik pada kelas luminositas spektral tertentu maupun pada tahap dalam evolusi bintang.

Bibliografi

Vassiliadis, E.; Wood, P. R. (1993). "Evolution of low- and intermediate-mass stars to the end of the asymptotic giant branch with mass loss". Astrophysical Journal. 413: 641. Bibcode:1993ApJ...413..641V. doi:10.1086/173033.
Pols, Onno R.; Schröder, Klaus-Peter; Hurley, Jarrod R.; Tout, Christopher A.; Eggleton, Peter P. (1998). "Stellar evolution models for Z = 0.0001 to 0.03". Monthly Notices of the Royal Astronomical Society. 298 (2): 525. Bibcode:1998MNRAS.298..525P. doi:10.1046/j.1365-8711.1998.01658.x .
Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C. (2000). "Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M?, and from Z=0.0004 to 0.03". Astronomy and Astrophysics Supplement Series. 141 (3): 371. arXiv:astro-ph/9910164 . Bibcode:2000A&AS..141..371G. doi:10.1051/aas:2000126.

@@ Baris 7: / Baris 7: @@
 * {{cite journal|bibcode= 2000A&AS..141..371G|doi=10.1051/aas:2000126|title=Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M?, and from Z=0.0004 to 0.03|journal=Astronomy and Astrophysics Supplement Series|volume=141|issue=3|pages=371|year=2000|last1=Girardi|first1=L.|last2=Bressan|first2=A.|last3=Bertelli|first3=G.|last4=Chiosi|first4=C.|arxiv = astro-ph/9910164 }}
 [[Kategori:Bintang]]
+[[Kategori:Jenis bintang]]