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19982007
most citedArgon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars

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astro-ph200740 cited

Argon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars

Thierry Lanz, Katia Cunha, Jon Holtzman +1

Argon abundances have been derived for a sample of B main-sequence stars in the Orion association. The abundance calculations are based on NLTE metal line-blanketed model atmospher…

astro-ph2006

A Grid of NLTE Line-Blanketed Model Atmospheres of Early B-type Stars

Thierry Lanz, Ivan Hubeny

We have constructed a comprehensive grid of 1540 metal line-blanketed, NLTE, plane-parallel, hydrostatic model atmospheres for the basic parameters appropriate to early B-type star…

astro-ph2005

Effects of mass loss for highly-irradiated giant planets

W. B. Hubbard, M. F. Hattori, A. Burrows +2

We present calculations for the evolution and surviving mass of highly-irradiated extrasolar giant planets (EGPs) at orbital semimajor axes ranging from 0.023 to 0.057 AU using a g…

astro-ph2005

Preliminary analysis of an extreme helium sdO star: BD+25 4655

J. Budaj, V. Elkin, I. Hubeny

Preliminary analysis of CCD spectra obtained by the 6m SAO telescope is presented. We have used simple H-He NLTE model atmospheres computed by TLUSTY to derive the basic parameters…

astro-ph2002

A New Formation Mechanism for the Hottest Horizontal-Branch Stars

Allen V. Sweigart, Thomas M. Brown, Thierry Lanz +2

Stars with very large mass loss on the red-giant branch can undergo the helium flash while descending the white-dwarf cooling curve. Under these conditions the flash convection zon…

astro-ph2000

Heavy element abundances in DA white dwarfs

M. A. Barstow, M. R. Burleigh, N. P. Bannister +4

We present a series of systematic abundance measurements for a group of hot DA white dwarfs in the temperature range 20,000-75,000K, based on far-UV spectroscopy with STIS on HST,…