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

Ishida M.; Morio K.; Ueda Y.

Vol. 20 No. 1 (2004), Contributions

Vol. 20 No. 1 (2004)

Contributions

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

Ishida M.⁺⁻
Morio K.⁺⁻
Ueda Y.⁺⁻

Ishida M.

Tokyo Metropolitan University, Japan.

Morio K.

-

Ueda Y.

-

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Keywords

stars: individual (CI CAM
XTE J0421+560)
X-rays: stars

How to Cite

Possibility of a White Dwarf as the Accreting Compact Star in CI Cam (XTE J0421+560). (2004). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 20(1), 104-105. https://astronomia.unam.mx/journals/rmxac/article/view/2004rmxac..20..104i

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Abstract

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

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