Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-12-23
Astronomy and Astrophysics
Astrophysics
4 pages, 1 figure, Accepted by A&A
Scientific paper
We have obtained high resolution optical spectroscopy of the accretion disc corona source 2S0921--630 (=V395 Car) that constrains the spectral type of the companion star to be most probably K0III. At 6500A the secondary star is found to contribute ~25% to the observed flux. The absorption line spectrum of the K0III companion star is broadened (compared to template stars) by a projected rotational velocity of 65+/-9 km/s (1 sigma).
Casares Jorge
Charles Phil A.
der Hooft Frank van
Kuulkers Eric
Paradijs Jan van
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