Results 121 to 130 of about 20,344 (216)
Unraveling Year-Long Radial Velocity Variations in Red Clump Region -- I: Comprehensive analysis of a K0 Giant star, 2 Draconis [PDF]
Udomlerd Srisuchinwong +20 more
openalex +2 more sources
We examined the double red clump (RC) observed in the Galactic bulge, interpreted as a difference in distance (“X-shaped bulge scenario”) or in chemical composition (“multiple population scenario”).
Seungsoo Hong +2 more
doaj +1 more source
Current observations indicate that stars with higher rotation rates appear to maintain more surface lithium, and the majority of lithium-rich giants are indeed red clump stars.
Xue-Feng Li +4 more
doaj +1 more source
Measurements of streaming motions of the Galactic bar with Red Clump Giants
T. Sumi, L. Eyer, P. R. Woźniak
openalex +1 more source
Many Roads Lead to Lithium: Formation Pathways For Lithium-rich Red Giants
Stellar models predict that lithium (Li) inside a star is destroyed during the first dredge-up phase, yet 1.2% of red giant stars are Li-rich. We aim to uncover possible origins of this population, by analyzing 1099 Li-rich giants ( A (Li) ≥ 1.5) in ...
Maryum Sayeed +10 more
doaj +1 more source
Fine structure of the red giant clump from Hipparcos data, and distance determinations based on its mean magnitude [PDF]
L. Girardi +3 more
openalex +1 more source
Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo?
We analyze the outer regions of M33, beyond 15 kpc in projected distance from its center, using Subaru/Hyper Suprime-Cam multicolor imaging. We identify red giant branch (RGB) stars and red clump (RC) stars using the surface-gravity-sensitive NB515 ...
Itsuki Ogami +10 more
doaj +1 more source
In the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology.
Marc H. Pinsonneault +40 more
doaj +1 more source
History of two mass loss processes in VY CMa. [PDF]
Quintana-Lacaci G +6 more
europepmc +1 more source
Distance estimates to five open clusters based on
Li Chen, Xinhua Gao
openalex +1 more source

