Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-23T20:25:45.157Z Has data issue: false hasContentIssue false
  • English
  • Français

BBXRT Observations of Supernova Remnants

Published online by Cambridge University Press:  30 March 2016

R. Petre ,
P. J. Serlemitsos ,
F. E. Marshall ,
K. Jahoda ,
E. A. Boldt ,
S. S. Holt ,
R. F. Mushotzky ,
J. Swank ,
A.E. Szymkowiak  and
R. Kelley
...Show all authors
R. Petre
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
P. J. Serlemitsos
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
F. E. Marshall
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
K. Jahoda
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
E. A. Boldt
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
S. S. Holt
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
R. F. Mushotzky
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
J. Swank
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
A.E. Szymkowiak
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
R. Kelley
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
A. Smale
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
K. Arnaud
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA
K. Weaver
Affiliation:
Code 666, Laboratory for High Energy Astrophysics NASA / Goddard Space Flight CenterGreenbelt, Maryland 20771USA

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.

The BBXRT observed nine supernova remnants during its nine-day flight. We present preliminary results from some of these observations, emphasizing the ability of BBXRT to perform spatially resolved spectroscopy. The improved spectral resolution and efficiency over previous instruments makes possible measurements of previously undetectable lines, and the broad bandpass allows simultaneous measurement of lines from oxygen through iron.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 229 - 233
Copyright
Copyright © Kluwer 1992

References

Fahlman, G.G., and Gregory, P.C. (1981), “An X-Ray Pulsar in SNR G109.1-1.0”, Nature, 293, 202–204.Google Scholar
Gregory, P.C., and Fahlman, G.G. (1980), “An Extraordinary New Celestial X-Ray Source”, Nature, 287, 805–807.Google Scholar
Hamilton, A.J.S., Sarazin, C.L., and Chevalier, R.A. (1983) “X-Ray Line Emission from Supernova Remnants. I. Models for Adiabatic Remnants”, Ap. J. (Suppl.), 51, 115–148.CrossRefGoogle Scholar
Hamilton, A.J.S., Sarazin, C.L., and Szymkowiak, A.E. (1986) “The X-Ray Spectrum of Tycho”, Ap. J., 300, 713–721.Google Scholar
Morini, M., Robba, N.R., Smith, A., and van der Klis, M. (1988) “EXOSAT Observations of the Supernova Remnant G109.1-1.0 and the X-Ray Pulsar IE 2259+589”,Ap. J., 333, 777–787.Google Scholar
Petre, R., Szymkowiak, A.E., Seward, F.D., and Willingale, R. (1988) “A Comprehensive Study of the X-Ray Structure and Spectrum of IC 443”, Ap. J., 335, 215–238.CrossRefGoogle Scholar
Serlemitsos, P., et al. (1991) “First Results from BBXRT”, Proc. of 21st Yamada Conference, in press.Google Scholar