Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...443..281j&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 443, no. 1, p. 281-294
Astronomy and Astrophysics
Astronomy
19
Asymptotic Giant Branch Stars, Carbon Stars, Chromosphere, Stellar Mass, Stellar Winds, Ultraviolet Astronomy, Ultraviolet Spectra, Velocity Distribution, Fluorescence, Hubble Space Telescope, Photosphere, Stellar Envelopes
Scientific paper
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 troposphere, 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.
Alexander David R.
Avrett Eugene H.
Brown Alexander
Carpenter Kenneth G.
Ensman Lisa M.
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