Hostname: page-component-f554764f5-sl7kg Total loading time: 0 Render date: 2025-04-10T06:24:03.770Z Has data issue: false hasContentIssue false
  • English
  • Français

Far-ultraviolet Emission from Supernova Remnant Shocks

Published online by Cambridge University Press:  25 May 2016

R. Sankrit ,
W. P. Blair  and
Fuse Snr Team
R. Sankrit
Affiliation:
Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, U.S.A.
W. P. Blair
Affiliation:
Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, U.S.A.
Fuse Snr Team
Affiliation:
JHU, Princeton, GSFC, IAP, UC Berkeley

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.

Supernova remnant shocks produce a rich spectrum of lines in the ultraviolet. Among these are important diagnostic resonance lines of O VI, C III, and N III which lie in the bandpass observable with the recently launched Far Ultraviolet Spectroscopic Explorer. We present an overview of a PI program to observe several supernova remnants using this new telescope.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 425 - 426
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Blair, W. P., Sankrit, R., Raymond, J. C., & Long, K. S. 1999, AJ, 118, 942.CrossRefGoogle Scholar
Levenson, N. A., Graham, J. R., Keller, L. D., & Richter, M. J. 1998, ApJS, 118, 541.CrossRefGoogle Scholar
Sankrit, R. & Hester, J. J. 1997, ApJ, 491, 796.Google Scholar