| Issue |
A&A
Volume 372, Number 2, June III 2001
|
|
|---|---|---|
| Page(s) | 563 - 565 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20010526 | |
| Published online | 15 June 2001 | |
On the orbital period of the cataclysmic variable RZ Leonis
1
Dpto. de Fisica, Facultad de Ciencias Fisicas y Matematicas, Universidad de Concepcion, Casilla 160-C, Concepcion, Chile
2
Dipartimento di Astronomia, Universita di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy e-mail: ctappert@pd.astro.it
Corresponding author: R. E. Mennickent, rmennick@stars.cfm.udec.cl
Received:
12
March
2001
Accepted:
4
April
2001
We present a time-resolved study of the Balmer emission lines of RZ Leo. From the analysis of the radial velocities we find an orbital period of 0.07651(26) d.
Key words: stars: individual: RZ Leonis / stars: novae, cataclysmic variables / stars: fundamental parameters / stars: evolution / binaries: general
© ESO, 2001
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