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Point X-Ray Sources in the Supernova Remnant RCW 86

Published online by Cambridge University Press:  26 May 2016

Vasilii V. Gvaramadze  and
Alexey A. Vikhlinin
Vasilii V. Gvaramadze
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij Pr. 13, Moscow, 119992, Russia
Alexey A. Vikhlinin
Affiliation:
Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow, 117997, Russia

Abstract

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We have discovered two point X-ray sources in the southwest protrusion of the supernova remnant (SNR) RCW 86. One of them is interpreted as a foreground active star, while the second one as a candidate neutron star associated with the SNR.

Type
Part 4 Supernovae and Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 145 - 146
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Gvaramadze, V.V. 2002, in New Visions of the X-ray Universe in the XMM-Newton and Chandra Era, ed. Jansen, F. (ESA SP-488), in press (astro-ph/0208028) Google Scholar
Gvaramadze, V.V., & Vikhlinin, A.A. 2003, A&A, in press (astro-ph/0208030) Google Scholar