A Classical Nova, V2487 Oph 1998, Seen in X-rays Before and After Its Explosion-Reference-Cited by-同舟云学术

A Classical Nova, V2487 Oph 1998, Seen in X-rays Before and After Its Explosion

Published:2002-10-11 Issue:5592 Volume:298 Page:393-395
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Hernanz Margarita¹,Sala Glòria¹

Affiliation:

1. Institut d'Estudis Espacials de Catalunya and Instituto de Ciencias del Espacio, Consejo Superior de Investigaciones Científicas, Gran Capità 2-4, E-08034 Barcelona, Spain.

Abstract

Classical nova explosions are very energetic and frequent phenomena caused by explosive hydrogen burning on top of an accreting white dwarf. Observations of the recent nova V2487 Oph 1998 by the X-ray Multi-Mirror satellite (XMM-Newton) provide evidence that accretion (probably on a magnetic white dwarf) was reestablished as early as 2.7 years after the explosion. In addition, positional correlation with a source previously discovered by the Röntgen Satellite (ROSAT) in 1990 suggests that the site of a nova explosion had been seen in x-rays before the outburst.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference36 articles.

1. S. Nakano K. Takamizawa R. Kushida Y. Kushida T. Kato Int. Astron. Union Circ. 6941 (1998).

2. A. V. Filippenko et al. Int. Astron. Union Circ. 6943 (1998).

3. Liller W., Jones A., Inform. Bull. Var. Stars 4870, 1 (2000).

4. Krautter J., Ögelman H., Starrfield S., Wichmann R., Pfeffermann E., Astrophys. J. 456, 788 (1996).

5. Ögelman H., Orio M., Krautter J., Starrfield S., Nature 361, 331 (1993).

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