SIMBAD references

2002A&A...382..554A - Astronomy and Astrophysics, volume 382, 554-555 (2002/2-1)

Support for a white dwarf in the Be star binary γ Cassiopeiae.

APPARAO K.M.V.

Abstract (from CDS):

The recently discovered orbital period for γ Cas and the modulation period in X-rays and optical are consistent with the orbital period-spin period relation for white dwarfs derived from a similar relation found for Be star - neutron star binaries. This lends support for the existence of a white dwarf in the γ Cas binary.

Abstract Copyright: ∼

Journal keyword(s): stars: γ Cas - white dwarf - stars: emission line, Be stars - stars: binaries - stars: neutron

Simbad objects: 3

Full paper

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