Ariel 1118-61 - A very close binary system or a slowly rotating neutron star

Details Ariel 1118-61 - A very close binary system or a slowly rotating neutron star Ariel 1118-61 - A very close binary system or a slowly rotating neutron star

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..42..161f&link_type=abstract

(COSPAR, Symposium on Fast Transients in X- and Gamma-Rays, Varna, Bulgaria, May 29-31, 1975.) Astrophysics and Space Science, v

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Neutron Stars, Stellar Models, Stellar Rotation, X Ray Sources, Light Curve, M Stars, Mass Transfer, Mira Variables, Orbital Elements, Periodic Variations, Variable Stars, X Ray Astronomy

Scientific paper

The transient X-ray source Ariel 1118-61 has a period of 6.75 min. We
review possible models for the X-ray source and in particular we
consider orbital and rotational origins for the periodicity. Finally we
discuss the possible identification of Ariel 1181-61 with the Mira-type
variable RS Cen.

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