activity
19972008
most citedThe influence of chemical composition on the properties of Cepheid stars. II-The iron content

227 citations · 1.1k across the 19 of their papers we have counts for

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Showing 2006Show all

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astro-ph2006

AGB stars in extragalactic systems

M. A. T. Groenewegen

I will be reviewing three methods to identify late-type giants in extragalactic systems, based on the main characteristics of AGB stars (they are infrared bright, variable, and hav…

astro-ph200682 cited

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud

Eric Lagadec, Albert A. Zijlstra, G. C. Sloan +12

We present Spitzer Space telescope spectroscopic observations of 14 carbon-rich AGB stars in the Small Magellanic Cloud. SiC dust is seen in most of the carbon-rich stars but it is…

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-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-ph2006181 cited

Near-Infrared Photometry of Carbon Stars

Patricia A. Whitelock, Michael W. Feast, Freddy Marang +1

Near-infrared, JHKL, photometry of 239 Galactic carbon-rich variable stars is presented and discussed. From these and published data the stars were classified as Mira or non-Mira v…

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…