Non-Radial Pulsations from RX J0105.1-7211

Details Non-Radial Pulsations from RX J0105.1-7211 Non-Radial Pulsations from RX J0105.1-7211

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..648....1s&link_type=abstract

The Astronomer's Telegram, #648

Astronomy and Astrophysics

Astronomy

4

Optical, X-Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

RX J0105.1-7211 (SXP3.34) is a Be/neutron-star binary in the Small Magellanic Cloud. It has one of the shortest pulsation periods among the many SMC Be/pulsar systems. The optical counterpart is #1506 from the emission-line catalogue of Meyssonnier & Azzopardi (1993, A&AS, 102, 451). In addition Coe et al. (2005, MNRAS, 356, 502) have shown that it has very strong H-alpha emission. They found a photometric period of 11.09 days, which they suggested was the orbital period, but found this to be inconsistent with the strength of the emission.

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