Results 31 to 40 of about 20,344 (216)
Metallicity of Red Clump Giants in Baade's Window [PDF]
8 pages, self-contained latex, 5 postscript figures, submitted to Acta ...
B. Paczyński
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Measurements of streaming motions of the Galactic bar with red clump giants [PDF]
7 pages, 9 figures, submitted to ...
T. Sumi, L. Eyer, P. R. Woźniak
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Modeling the Galactic Bar Using Red Clump Giants [PDF]
submitted to the New Astronomy, 27 pages, 11 figures; also available at ftp://www.astro.princeton.edu/stanek/Barmodel and through WWW at http://www.astro.princeton.edu/~library/prep ...
Stanek, K. Z. +6 more
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The abundances of nearby red clump giants [PDF]
Abstract Based on the analysis of high-resolution spectra with a high signal-to-noise ratio, we have determined the abundances of the α-elements O, Si, Ca and Ti, the iron peak elements V, Fe and Ni, and the heavy element Ba without the consideration of non-local thermodynamic equilibrium (NLTE) effect and the light neutron-rich elements
Y. J. Liu +4 more
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A secondary clump of red giant stars: why and where [PDF]
20 pages with 11 figures, submitted to ...
L. Girardi
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Tracing the long bar with red-clump giants [PDF]
16 pages, 35 figures, accepted for publication in A& ...
Cabrera-Lavers, A. +5 more
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Spectroscopic and Asteroseismic Analysis of the Secondary Clump Red Giant HD 226808* [PDF]
Abstract In order to clarify the properties of the secondary clump star HD 226808 (KIC 5307747), we combined four years of data from Kepler space photometry with high-resolution spectroscopy of the High Efficiency and Resolution Mercator Échelle Spectrograph mounted on the Mercator telescope.
Bruno Lustosa de Moura +8 more
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The GALAH survey: velocity fluctuations in the Milky Way using Red Clump giants [PDF]
20 pages, 16 figures, accepted for publication in ...
S. Khanna +22 more
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A LITHIUM-RICH RED GIANT BELOW THE CLUMP IN THE KEPLER CLUSTER, NGC 6819 [PDF]
WIYN/HYDRA spectra in the Li 6708 Angstrom region have been obtained for 332 probable members of the old open cluster, NGC 6819. Preliminary analysis shows a pattern of Li depletion from the top of the turnoff to the base of the giant branch. Starting one magnitude below the level of the clump, all brighter giants have A(Li) below 1.0, with most having
Barbara J. Anthony-Twarog +3 more
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Red clump giant stars as tracers of Galactic structure [PDF]
AbstractBy isolating the red clump giant population in the color-magnitude diagrams and inverting their star counts, we can obtain directly the density distribution of the old stellar population along the line of sight. We have applied this method to several near infrared surveys and obtained information on the disc, bulge and long bar.
M. López-Corredoira +5 more
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