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 language | English |
|---|---|
| Pages (from-to) | 281-294 |
| Number of pages | 14 |
| Journal | Astrophysical Journal |
| Volume | 443 |
| Issue number | 1 |
| DOIs | |
| State | Published - Apr 10 1995 |
Keywords
- Stars: carbon
- Stars: chromospheres
- Stars: mass loss
- Ultraviolet: stars