Hostname: page-component-848d4c4894-ttngx Total loading time: 0 Render date: 2024-05-21T00:10:01.128Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  22 February 2018

Manabu Ishida ,
Kazuyuki Morio  and
Yoshihiro Ueda
Manabu Ishida
Affiliation:
Tokyo Metropolitan University, Japan
Kazuyuki Morio
Affiliation:
ISAS/JAXA, Japan
Yoshihiro Ueda
Affiliation:
ISAS/JAXA, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Resumen

Resumen

Aunque CI Cam, la cual presentó una explosión en abril de 1998, ha sido considerada como una fuente transitoria de ray os X suaves (SXT) que alberga un agujero negro, posee a la vez ciertas características que difícilmente pueden hacerla encajar dentro del grupo de SXT. En este artículo proponemos una enana blanca como la estrella central acreciente en CI Cam.

Keywords

StarsIndividual (CI Cam, XTE J0421+560) — X-RaysStars
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 104 - 105
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Asai, K., Dotani, T., Hoshi, R., Tanaka, Y., Robinson, С. R., & Terada, K. 1998b, PASJ, 50, 611 CrossRefGoogle Scholar
Belloni, T., et al. 1999, ApJ, 527, 345 CrossRefGoogle Scholar
Cohen, J. G. 1988, in ASP Conf. Ser. 4, The Extra-galactic Distance Scale, ed. Bergh, S. van den & Pritchet, C. J. (San Francisco: ASP), 114 Google Scholar
Ebisawa, K., Mukai, K., Kotani, T., Asai, K., Dotani, T., Nagase, F., Hartmann, H. W., Heise, J., Kahabka, P., & van Teeseling, A. 2001, /apj, 550, 1007 Google Scholar
Frontera, A. et al. 1998, A&A, 339, L69 Google Scholar
Hynes, R. I., et al. 2002, A&A, 392, 991 Google Scholar
Ishida, M., Morio, K., & Ueda, Y. 2004, ApJ, 601, in press CrossRefGoogle Scholar
Krautter, J., Ögelman, H., Starrfield, S., Wichmann, W., & Pfeffermann, E. 1996, ApJ, 456, 788 CrossRefGoogle Scholar
Orio, M., Parmar, A. N., Greiner, J., Ögelman, H., Starrfield, S., & Trussoni, E. 2002, MNRAS, 333, L11 Google Scholar
Orr, A., Parmar, A. N., Orlandini, M., Frontera, A., Dal Fiume, D., Segreto, A., Santangelo, A., & Tavani, M. 1998, A&A, 340, L19 Google Scholar
Robinson, E. L., Ivans, I. I., & Welsh, W. F. 2002, ApJ, 565, 1169 Google Scholar
Smith, D., Remillard, R., Swank, J., Takeshima, T., & Smith, E. 1998, IAU Circ., 6855 Google Scholar
Starrfield, S., et al. 2000, BAAS, 32, 4103 Google Scholar
Ueda, Y., Ishida, M., Inoue, H., Dotani, T., Greiner, J., & Lewin, W. H. G. 1998, ApJ, 508, L167 Google Scholar