activity
19992009
most citedAGB stars in the Magellanic Clouds. II. The rate of star formation across the LMC

141 citations · 520 across the 7 of their papers we have counts for

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15 papers · 1 filter

astro-ph200720 cited

Near-Infrared photometry of carbon stars in the Sagittarius dwarf irregular galaxy and DDO 210

M. Gullieuszik, M. Rejkuba, M. R. Cioni +2

We investigate the intermediate-age asymptotic giant branch stellar population of two Local Group dwarf irregular galaxies to characterize their carbon star population in near-infr…

astro-ph200633 cited

ISO Mid-Infrared Spectroscopy of Galactic Bulge AGB Stars

Joris A. D. L. Blommaert, Martin A. T. Groenewegen, Koryo Okumura +8

To study the nature of Bulge AGB stars and in particular their circumstellar dust, we have analysed mid-infrared spectra obtained with the ISOCAM CVF spectrometer in three Bulge fi…

astro-ph2006117 cited

Lithium and zirconium abundances in massive Galactic O-rich AGB stars

D. A. Garcia-Hernandez, P. Garcia-Lario, B. Plez +4

Lithium and zirconium abundances (the latter taken as representative for s-process enrichment) are determined for a large sample of massive Galactic O-rich AGB stars, for which hig…

astro-ph200679 cited

Spitzer observations of acetylene bands in carbon-rich AGB stars in the Large Magellanic Cloud

M. Matsuura, P. R. Wood, G. C. Sloan +13

We investigate the molecular bands in carbon-rich AGB stars in the Large Magellanic Cloud (LMC), using the InfraRed Spectrograph (IRS) on board the Spitzer Space Telescope (SST) ov…

astro-ph2006126 cited

A Spitzer mid-infrared spectral survey of mass-losing carbon stars in the Large Magellanic Cloud

Albert A. Zijlstra, Mikako Matsuura, Peter R. Wood +13

We present a Spitzer Space Telescope spectroscopic survey of mass-losing carbon stars (and one oxygen-rich star) in the Large Magellanic Cloud. The spectra cover the wavelength ran…

astro-ph2005

Why are massive O-rich AGB stars in our Galaxy not S-stars?

D. A. Garcia-Hernandez, P. Garcia-Lario, B. Plez +4

We present the main results derived from a chemical analysis carried out on a large sample of galactic O-rich AGB stars using high resolution optical spectroscopy (R~40,000-50,000)…