Possibility of a White Dwarf as the Accreting Compact Star in CI Cam (XTE J0421+560)

Details Possibility of a White Dwarf as the Accreting Compact Star in CI Cam (XTE J0421+560) Possibility of a White Dwarf as the Accreting Compact Star in CI Cam (XTE J0421+560)

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..104i&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

Stars: Individual (Ci Cam, Xte J0421+560), X-Rays: Stars

Scientific paper

Although CI Cam, which showed an outburst in April 1998, has been
regarded as a soft X-ray transient (SXT) harboring a black hole, it has
some characteristics that can hardly be reconciled with the SXT picture.
In this paper, we propose a white dwarf as the central accreting star in
CI Cam.

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