High-resolution spectra of stars in globular clusters. VI - Oxygen-deficient red giant stars in M13

1991 ◽  
Vol 101 ◽  
pp. 1693 ◽  
Author(s):  
Jeffery A. Brown ◽  
George Wallerstein ◽  
J. B. Oke
2013 ◽  
Vol 9 (S301) ◽  
pp. 325-331 ◽  
Author(s):  
S. Hekker ◽  
A. Mazumdar

AbstractThanks to significant improvements in high-resolution spectrographs and the launch of dedicated space missions MOST, CoRoT and Kepler, the number of subgiants and red-giant stars with detected oscillations has increased significantly over the last decade. The amount of detail that can now be resolved in the oscillation patterns does allow for in-depth investigations of the internal structures of these stars. One phenomenon that plays an important role in such studies are mixed modes. These are modes that carry information of the inner radiative region as well as from the convective outer part of the star allowing to probe different depths of the stars.Here, we describe mixed modes and highlight some recent results obtained using mixed modes observed in subgiants and red-giant stars.


2009 ◽  
Vol 5 (S268) ◽  
pp. 361-362
Author(s):  
Laimons Začs ◽  
Arturs Barzdis

AbstractThe lithium abundance was calculated for five metal-poor red giant stars from Li i doublet at 6707 Å by fitting the observed high-resolution spectra with synthetic spectra. The lithium abundance was found to be low in all stars, logϵ(Li) ≤ 1.8, confirming lithium depletion on the red giant and asymptotic giant branch.


2006 ◽  
Vol 640 (2) ◽  
pp. 801-822 ◽  
Author(s):  
Jennifer A. Johnson ◽  
Inese I. Ivans ◽  
Peter B. Stetson

Nature ◽  
1969 ◽  
Vol 224 (5223) ◽  
pp. 1006-1008 ◽  
Author(s):  
ICKO IBEN ◽  
ROBERT T. ROOD ◽  
KAREN M. STROM ◽  
STEPHEN E. STROM

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