The X-ray light curve of 4U 2129+47

Details The X-ray light curve of 4U 2129+47 The X-ray light curve of 4U 2129+47

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l.159u&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Feb. 1, 1980, p. L159-L161.

Astronomy and Astrophysics

Astrophysics

15

Binary Stars, Light Curve, Stellar Models, X Ray Sources, Dwarf Stars, M Stars, Neutron Stars

Scientific paper

The light curve of 4U 2129+47 is presented showing that it almost
certainly has a period of approximately 0.22 days. This is the same
period as the optical candidate proposed by Thorstensen et al. (1979).
Binary X-ray source models, consisting of an M dwarf plus either a
neutron star or a white dwarf, are briefly discussed.

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