The red clump is a clustering of red giants in the Hertzsprung–Russell diagram at around 5,000 K and absolute magnitude (MV) +0.5, slightly hotter than... 13 KB (1,655 words) - 05:01, 5 February 2024 |
bars, one nestled within the other. The bar is delineated by red-clump stars (see also red giant); however, RR Lyrae variables do not trace a prominent... 48 KB (4,911 words) - 02:27, 26 April 2024 |
was confirmed by the same means, by core helium-burning red clump stars, and by the tip of the red giant branch. All three papers find an inclination of... 33 KB (3,564 words) - 08:47, 26 April 2024 |
descriptions as a fallback Hess diagram – Diagram of stars in astronomy Red clump – Clustering of stars in astronomy diagram Stellar birthline – Construct... 23 KB (2,771 words) - 02:01, 9 April 2024 |
Stellar evolution (section Red-giant-branch phase) are often observed as a red clump of stars in the colour-magnitude diagram of a cluster, hotter and less luminous than the red giants. Higher-mass stars... 49 KB (6,424 words) - 20:50, 5 March 2024 |
times the Sun's luminosity and 11.98 ± 0.57 times its radius. An aging red clump star, it is fusing helium to carbon and oxygen in its core. Capella Ab... 71 KB (7,622 words) - 11:46, 15 March 2024 |
mixed traits of an evolved subgiant and giant star. It is catalogued as a red clump giant, which would indicate it is generating energy through helium fusion... 8 KB (623 words) - 12:40, 27 July 2023 |
the VVV survey with the help of red clump stars. The VVV survey also found two overlapping populations of red clump stars and an X-shape of the bulge... 17 KB (1,936 words) - 19:13, 13 April 2024 |
class of star that develops from a red dwarf after it has exhausted much of its hydrogen fuel supply. Because red dwarfs fuse their hydrogen slowly and... 4 KB (545 words) - 13:59, 15 December 2023 |
measured CP of q = 7 × 10 − 3 {\displaystyle q=7\times 10^{-3}} for the red supergiant NML Cygni and q = 2 × 10 − 3 {\displaystyle q=2\times 10^{-3}}... 14 KB (1,695 words) - 16:59, 24 February 2024 |
object Hayashi track Henyey track Evolution Main sequence Red-giant branch Horizontal branch Red clump Asymptotic giant branch post-AGB super-AGB Blue loop... 7 KB (415 words) - 21:15, 17 April 2023 |
Giant star (section Red giants) their lives: a main red-giant branch (RGB); a red horizontal branch or red clump; the asymptotic giant branch (AGB), although AGB stars are often large... 16 KB (2,321 words) - 14:49, 20 April 2024 |
giant branch Hess diagram Red clump Stellar classification Müller, Oliver; Rejkuba, Marina; Jerjen, Helmut (2018). "Tip of the red giant branch distances... 6 KB (640 words) - 15:38, 19 October 2023 |
object Hayashi track Henyey track Evolution Main sequence Red-giant branch Horizontal branch Red clump Asymptotic giant branch post-AGB super-AGB Blue loop... 9 KB (967 words) - 08:10, 11 March 2024 |
clumping of particles. The word agglutination comes from the Latin agglutinare (glueing to). Agglutination is a reaction in which particles (as red blood... 5 KB (547 words) - 14:24, 10 January 2024 |
Look up red dwarf in Wiktionary, the free dictionary. Wikimedia Commons has media related to Red dwarfs. This is a list of exceptional red dwarfs. This... 17 KB (839 words) - 15:15, 5 March 2024 |
luminosity class V: main-sequence stars (dwarfs). Example: Achernar (B6Vep) Red dwarfs are low-mass main-sequence stars. Yellow dwarfs are main-sequence... 5 KB (579 words) - 20:08, 17 February 2024 |
using the Spitzer Space Telescope failed to show the expected density of red clump giants in the direction of the Sagittarius and Norma arms. In January... 5 KB (558 words) - 20:19, 11 January 2024 |