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DUST IS FORMING ALONG THE RED GIANT BRANCH OF 47 TucThis work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech.
Online Contents | 2010| -
The First Detailed Abundances for M giants in Baade's Window from Infrared Spectroscopy
Free accessArXiv | 2005| -
A NEAR-INFRARED SPECTROSCOPIC SCREENING OF THE RED GIANT POPULATIONS IN w CENTAURI
Online Contents | 2003| -
ISOCAM OBSERVATIONS OF GALACTIC GLOBULAR CLUSTERS: MASS LOSS ALONG THE RED GIANT BRANCH
Online Contents | 2002| -
HIGH-RESOLUTION INFRARED SPECTRA OF BULGE GLOBULAR CLUSTERS: LILLER I AND NGC 6553
Online Contents | 2002| -
Abundance analysis in the near IR: stellar clusters and galaxies
National licenceSpringer Verlag | 2001| -
EVOLUTIONARY SYNTHESIS MODELING OF RED SUPERGIANT FEATURES IN THE NEAR-INFRARED
Online Contents | 1999| -
The First Detailed Abundances for M giants in the inner Bulge from Infrared Spectroscopy
Free accessArXiv | 2007|
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