Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/730
Title: Circumstellar features in hot DA white dwarfs
Authors: Bannister, N. P.
Barstow, Martin A.
Holberg, J. B.
Bruhweiler, F. C.
First Published: 1-May-2003
Publisher: Oxford University Press (OUP), Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2003, 341 (2), pp.477-495
Abstract: We present a phenomenological study of highly ionized, non-photospheric absorption features in high spectral resolution vacuum ultraviolet spectra of 23 hot DA white dwarfs. Prior to this study, four of the survey objects (Feige 24, REJ 0457−281, G191−B2B and REJ 1614−085) were known to possess these features. We find four new objects with multiple components in one or more of the principal resonance lines: REJ 1738+665, Ton 021, REJ 0558−373 and WD 2218+706. A fifth object, REJ 2156−546, also shows some evidence of multiple components, though further observations are required to confirm the detection. We discuss possible origins for these features including ionization of the local interstellar environment, the presence of material inside the gravitational well of the white dwarf, mass loss in a stellar wind and the existence of material in an ancient planetary nebula around the star. We propose ionization of the local interstellar medium as the origin of these features in G191−B2B and REJ 1738+665, and demonstrate the need for higher-resolution spectroscopy of the sample, to detect multiple interstellar medium velocity components and to identify circumstellar features that may lie close to the photospheric velocity.
DOI Link: 10.1046/j.1365-8711.2003.06409.x
Links: http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2003.06409.x/abstract
http://hdl.handle.net/2381/730
Type: Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2003 Royal Astronomical Society Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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