STIS observations of five hot white dwarfs

Loading...
Thumbnail Image

Date

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

We present some early results from a study of five hot DA white dwarf stars, based on spectra obtained using STIS. All show multiple components in one or more of the strong resonance absorption lines typically associated with the stellar photosphere (e.g. C IV, Si IV, N V and O V). Possible relationships between the non-photospheric velocity components and the interstellar medium or local stellar environment, are investigated, including contributions from gravitational redshifting.
6 pages, 4 figures. 12th International Workshop on White Dwarf Stars (Delaware, USA)

Keywords

Citation

Collections

Endorsement

Review

Supplemented By

Referenced By