Bibcode
Lázaro, C.; Solheim, J. E.; Arévalo, M. J.
Referencia bibliográfica
Astrophysics and Space Science, Volume 169, Issue 1-2, pp. 259-261
Fecha de publicación:
7
1990
Revista
Número de citas
1
Número de citas referidas
1
Descripción
We present some preliminary results of a time-resolved spectroscopic
study of the peculiar cataclysmic system AM CVn. The analysis of He i
lines profile variability, suggests the existence of a 1051 s
periodicity. This is one of the known photometric periods, candidate to
be the orbital period of the system, or the rotational period of the
primary.