Massive Stars in Transition: Spectroscopic Analysis of HR Carinae

Details Massive Stars in Transition: Spectroscopic Analysis of HR Carinae Massive Stars in Transition: Spectroscopic Analysis of HR Carinae

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...77m&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Other

Stars: Emission-Line, Stars: Individual (Hr Carinae), Stars: Mass Loss, Stars: Variables: Other

Scientific paper

We analysed the high-resolution data of the LBV (or S Dor variable) HR
Carinae, taken with the FEROS spectrograph in the wavelength range 3900
to 8200 Å . We performed a spectral analysis of the Balmer lines
with a non-LTE expanding atmosphere code in order to derive its stellar
parameters and to infer its evolutive status.

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