Outer layers of a carbon star: The view from the Bubble Space Telescope

Hollis R. Johnson, Lisa M. Ensman, David R. Alexander, Eugene H. Avrett, Alexander Brown, Kenneth G. Carpenter, Kjell Eriksson, Bengt Gustafsson, Uffe G. Jørgensen, Philip D. Judge, Jeffrey L. Linsky, Donald G. Luttermoser, Francois Querci, Monique Querci, Richard D. Robinson, Robert F. Wing

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

To advance our understanding of the relationship between stellar chromospheres and mass loss, which is a common property of carbon stars and other asymptotic giant branch stars we have obtained ultraviolet spectra of the nearby N-type carbon star UU Aur using the Hubble Space Telescope (HST). In this paper we describe the HST observations, identify spectral features in both absorption and emission, and attempt to infer the velocity field in the chromosphere, upper photosphere, and circumstellar envelope from spectral line shifts. A mechanism for producing fluoresced emission to explain a previously unobserved emission line is proposed. Some related ground-based observations are also described.

Original languageEnglish
Pages (from-to)281-294
Number of pages14
JournalAstrophysical Journal
Volume443
Issue number1
DOIs
StatePublished - Apr 10 1995

Keywords

  • Stars: carbon
  • Stars: chromospheres
  • Stars: mass loss
  • Ultraviolet: stars

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