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High-resolution spectroscopy of G191-B2B in the extreme-ultraviolet

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posted on 2012-10-24, 09:04 authored by R.G. Cruddace, M.P. Kowalski, D. Yentis, C.M. Brown, H. Gursky, Martin A. Barstow, N.P. Bannister, G.W. Fraser, J.E. Spragg, J.S. Lapington, J.A. Tandy, B. Sanderson, J.L. Culhane, T.W. Barbee, J.F. Kordas, W. Goldstein, G.G. Fritz
We report a high-resolution (R = 3000-4000) spectroscopic observation of the DA white dwarf G191-B2B in the extreme-ultraviolet band 220-245 Å. A low-density, ionized He component is clearly present along the line of sight, which if completely interstellar implies a He ionization fraction considerably higher than is typical of the local interstellar medium. However, some of this material may be associated with circumstellar gas, which has been detected by analysis of the C IV absorption-line doublet in a Hubble Space Telescope/Space Telescope Imaging Spectrograph spectrum. A stellar atmosphere model assuming a uniform element distribution yields a best fit to the data that includes a significant abundance of photospheric He. The 99% confidence contour for the fit parameters excludes solutions in which photospheric He is absent, but this result needs to be tested using models allowing abundance gradients.

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Citation

ASTROPHYSICAL JOURNAL LETTERS, 2002, 565 (1), L47-L50.

Version

  • VoR (Version of Record)

Published in

ASTROPHYSICAL JOURNAL LETTERS

Publisher

IOP Publishing

issn

2041-8205

eissn

2041-8213

Copyright date

2002

Available date

2012-10-24

Publisher version

http://iopscience.iop.org/1538-4357/565/1/L47/

Language

en

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