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20042012
most citedDust driven mass loss from carbon stars as a function of stellar parameters - I. A grid of Solar-metallicity wind models

103 citations · 176 across the 7 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 65 cited

Intense Mass Loss from C-rich AGB Stars at low Metallicity?

L. Mattsson, R. Wahlin, S. Höfner +1

We argue that the energy injection of pulsations may be of greater importance to the mass-loss rate of AGB stars than metallicity, and that the mass-loss trend with metallicity is…

astro-ph2006★ 3 cited

The Chemical Composition of Red Giants, AGB Stars and Planetary Nebulae

Bengt Gustafsson, Rurik Wahlin

The determinations of element abundances in red-giant stars and in particular in AGB stars are reviewed and the resulting abundances are compared with those obtained for planetary…

astro-ph2006

Carbon stars in local group dwarf galaxies: C and O abundances

R. Wahlin, K. Eriksson, B. Gustafsson +4

We present abundances of carbon and oxygen as well as abundance ratios 12C/13C for a sample of carbon stars in the LMC, SMC, Carina, Sculptor and Fornax dwarf galaxies. The overall…

astro-ph2005

X-RED: A Satellite Mission Concept To Detect Early Universe Gamma Ray Bursts

Mirko Krumpe, Deirdre Coffey, Georg Egger +14

Gamma ray bursts (GRBs) are the most energetic eruptions known in the Universe. Instruments such as Compton-GRO/BATSE and the GRB monitor on BeppoSAX have detected more than 2700 G…

astro-ph2005★ 1 cited

Chemical analysis of carbon stars in the Local Group: I. The Small Magellanic Cloud and the Sagittarius dwarf spheroidal galaxy

P. De Laverny, C. Abia, I. Dominguez +5

We present the first results of our ongoing chemical study of carbon stars in the Local Group of galaxies. We used spectra obtained with UVES at the 8.2 m Kueyen-VLT telescope and…

astro-ph2004★ 4 cited

The Abundance of Elements in Cool Stars, as Determined from High-Resolution, 1-5 Micron Spectroscopy

N. Ryde, B. Gustafsson, K. Eriksson +1

We review the field of abundance determinations of elements in cool stars, with special interest paid to determinations based on analyses of high-resolution, 1-5 micron spectra. We…