Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-29T23:53:33.778Z Has data issue: false hasContentIssue false
  • English
  • Français

Chandra Studies of Supernova Remnants and Pulsars

Published online by Cambridge University Press:  13 May 2016

Patrick Slane ,
John P. Hughes ,
Cara E. Rakowski ,
David N. Burrows ,
John A. Nousek ,
Gordon P. Garmire  and
Bryan M. Gaensler
Patrick Slane
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
John P. Hughes
Affiliation:
Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019, USA
Cara E. Rakowski
Affiliation:
Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019, USA
David N. Burrows
Affiliation:
Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802, USA
John A. Nousek
Affiliation:
Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802, USA
Gordon P. Garmire
Affiliation:
Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802, USA
Bryan M. Gaensler
Affiliation:
Center for Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

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.

With sub-arcsecond angular resolution accompanied by fast time resolution and spatially resolved spectral capabilities, the Chandra X-ray Observatory provides a unique capability for the study of supernova remnants (SNRs) and pulsars. Though in its relative infancy, Chandra has already returned stunning images of SNRs which reveal the distribution of ejecta synthesized in the stellar explosions, the distinct properties of the forward and reverse shocks, and the presence of faint shells surrounding compact remnants. Pulsar observations have uncovered jet features as well as small-scaled structures in synchrotron nebulae. In this brief review we discuss results from early Chandra studies of pulsars and SNRs.

Type
Supernovae, Pulsars, and the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 358 - 365
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Chakrabarty, D., Pivovaroff, M. J., Hernquist, L. E., Heyl, J. S., & Narayan, R. 2001, to appear in ApJ, Vol. 546.Google Scholar
Ellison, D. C., Berezhko, , El, G., & Baring, M. G. 2000, ApJ, 540, 292.CrossRefGoogle Scholar
Flanagan, K. A. 2001 - to appear in Proc. of 11th Annual Oct. Astrophysics Conference in MD, Young Supernova Remnants, ed. Hwang, U. Google Scholar
Gaetz, T. J. et al. 2000, ApJ, 534, 47L.CrossRefGoogle Scholar
Gotthelf, E. V., & Wang, D. Q. 2000, ApJ, 532, L117.CrossRefGoogle Scholar
Hughes, J. P., Rakowski, C. E., Burrows, D. N., & Slane, P. O. 2000, ApJ, 528, L109.CrossRefGoogle Scholar
Hughes, J. P., Rakowski, C. E., & Decourchelle, A. 2000, ApJ, 543L, 61.Google Scholar
Hwang, U., Holt, S. S., & Petre, R. 2000, ApJ, 537, L119.CrossRefGoogle Scholar
Janka, H.-T., Müller, E. 1996, A&A, 306, 167.Google Scholar
Kennel, C. F., Coroniti, F. V. 1984, ApJ, 283, 710.CrossRefGoogle Scholar
Kifonidis, K., Plewa, T., Janka, H.-Th., & Müller, E. 2000, ApJ, 531, L123.CrossRefGoogle Scholar
Koyama, K. et al. 1995 Nature 378, 255.CrossRefGoogle Scholar
Koyama, K. et al. 1997, PASJ, 49, L7.CrossRefGoogle Scholar
Muraishi, H. et al. 2000, A&A, 354, L57.Google Scholar
Pavlov, G. G., Zavlin, V. E., Aschenbach, B., Trümper, J., & Sanwal, D. 2000, ApJ, 531, L53.CrossRefGoogle Scholar
Seward, F. D., & Wang, Z.-R. 1988, ApJ, 332, 199.CrossRefGoogle Scholar
Slane, P. et al. 1999, ApJ, 525, 357.CrossRefGoogle Scholar
Slane, P. et al. 2000, ApJ, 533, L29.CrossRefGoogle Scholar
Slane, P. et al. 2001, ApJ - accepted (see astro-ph/0010510).Google Scholar
Thielemann, F. K., Nomoto, K., & Hashimoto, M. 1996, ApJ, 460, 408.CrossRefGoogle Scholar
Torii, K., Tsunemi, H., & Slane, P. 1998, in IAU Symposium 188, The Hot Universe, ed. Koyama, K., Kitamoto, S., & Itoh, M. (Dordrecht: Kluwer Academic), 258.CrossRefGoogle Scholar
Warwick, R. S. et al. 2001, A&A - accepted (see astro-ph/0011245).Google Scholar
Weisskopf, M. C. et al. 2000, ApJ, 536, L81.CrossRefGoogle Scholar