Support for a white dwarf in the Be star binary gamma Cassiopeiae

Details Support for a white dwarf in the Be star binary gamma Cassiopeiae Support for a white dwarf in the Be star binary gamma Cassiopeiae

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...382..554a&link_type=abstract

Astronomy and Astrophysics, v.382, p.554-555 (2002)

Astronomy and Astrophysics

Astrophysics

2

Stars: Gamma Cas, White Dwarf, Stars: Emission Line, Be Stars, Stars: Binaries, Stars: Neutron

Scientific paper

The recently discovered orbital period for gamma 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 gamma Cas binary.

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