Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T04:17:15.823Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray properties of G308.3-1.4 and its central compact object

Published online by Cambridge University Press:  20 March 2013

K. A. Seo ,
C. Y. Hui ,
R. H. H. Huang ,
L. Trepl ,
T.-N. Lu ,
A. K. H. Kong  and
F. M. Walter
K. A. Seo
Affiliation:
Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea
C. Y. Hui
Affiliation:
Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea
R. H. H. Huang
Affiliation:
Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan
L. Trepl
Affiliation:
Astrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, Schillergäßchen 2-3, 07745 Jena, Germany
T.-N. Lu
Affiliation:
Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan
A. K. H. Kong
Affiliation:
Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan
F. M. Walter
Affiliation:
Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, USA
Rights & Permissions [Opens in a new window]

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.

We present a short Chandra observation that confirms a previous unidentified extended X-ray source, G308.3-1.4, as a new supernova remnant (SNR) in the Milky Way. Apart from identifying its SNR nature, a bright X-ray point source has also been discovered at the geometrical center. Its X-ray spectral properties are similar to those of a particular class of neutron star known as central compact objects (CCOs). On the other hand, the optical properties of this counterpart suggests it to be a late-type star. Together with the interesting ~ 1.4 hours X-ray periodicity found by Chandra, this system can possibly provide the first direct evidence of a compact binary survived in a supernova explosion.

Keywords

supernova remnantsX-rays
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 489 - 491
Copyright
Copyright © International Astronomical Union 2013

References

Bock, D., Large, M. I., & Sadler, E. M. 1999, AJ, 117, 1578Google Scholar
De Horta, A. Y., et al. 2012, arXiv:1210.2781v1Google Scholar
Hui, C. Y., et al. 2012, ApJ, 750, 7CrossRefGoogle Scholar
Hui, C. Y. & Becker, W. 2009, A&A, 494, 1005Google Scholar
Hui, C. Y. & Becker, W. 2006, A&A, 454, 543Google Scholar
Whiteoak, J. B. Z. 1992 A&A, 262, 251Google Scholar