A new correlation for Be/X-ray binaries: the orbital period-Hα equivalent width diagram.

Details A new correlation for Be/X-ray binaries: the orbital period-Hα equivalent width diagram. A new correlation for Be/X-ray binaries: the orbital period-Hα equivalent width diagram.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...322..193r&link_type=abstract

Astronomy and Astrophysics, v.322, p.193-196

Astronomy and Astrophysics

Astrophysics

53

Stars: Be, Stars: Neutron, X-Rays: Stars, Binaries: Close

Scientific paper

A correlation between the orbital period and the strength of the Hα line in Be/X-ray binaries has been found. Those systems with shorter orbital periods show less emission in Hα than those with longer orbital periods. The neutron star appears to act as a barrier which prevents the formation of a extended disk in systems with short orbital period.

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