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Optical and UV Observations of Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

Robert A. Fesen
Robert A. Fesen*
Affiliation:
Dartmouth College, Dept. of Physics and Astronomy, Hanover, NH 03755, USA

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Recent observations of the galactic supernova remnants the Crab Nebula, SN 1006, Cas A, and the Cygnus Loop are reviewed. New studies of the Crab Nebula suggest its progenitor may have had appreciable mass loss in the form of a circumstellar disk resulting in both a bipolar expansion and formation of the synchrotron ‘bays'. Unusually high proper motion knots near to and possibly directed away from the pulsar also have been reported. In the Cas A remnant, a NE jet of ejecta appears to be a plume of mantle material with expansion velocities up to 12000 km s-1 or nearly twice that seen in the main ejecta shell. HST observations of the sdOB star located behind SN 1006 indicate symmetrically expanding Fe II ejecta out to 8100 km s-1. Lastly, deep images of the Cygnus Loop reveal emission structures similar to those seen in 2D & 3D shocked cloud simulations.

Type
Supernova Remnants
Information
International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 381 - 389
Copyright
Copyright © Cambridge University Press 1996

References

Blair, W. P., Long, K. S., Vancura, O., Bowers, C. W., Conger, S., Davidsen, A. F., Kriss, G. A. & Henry, R. B. C. 1992, ApJ, 399, 611.Google Scholar
Chevalier, R. A. & Kirshner, R. P. 1979, ApJ, 233, 154.Google Scholar
Downes, R. A. & Fesen, R. A. 1993, in preparation.Google Scholar
Fesen, R. A. & Becker, R. H. 1991, ApJ, 371, 621.Google Scholar
Fesen, R. A., Kwitter, K. B., & Downes, R. A. 1992, AJ, 104, 719.Google Scholar
Fesen, R. A., Martin, C. L., & Shull, J. M. 1992, ApJ, 399, 599.Google Scholar
Fesen, R. A. & Staker, B. 1993, MNRAS, 263, 69.Google Scholar
Fesen, R. A., Wu, C.-C., Leventhal, M. & Hamilton, A. J. S. 1988, ApJ, 327, 164.Google Scholar
Gunderson, K., & Fesen, R. A. 1993, in preparation.Google Scholar
Henry, R. B. C. & MacAlpine, G. 1982, ApJ, 258, 11.Google Scholar
Hester, J. J. 1987, ApJ, 314, 187.Google Scholar
Klein, R. I., McKee, C. F. & Colella, P. 1991, In Supernovae, ed. Woosley, S. E. (Springer: New York) pp. 696.Google Scholar
MacAlpine, G. M., McGaugh, S. S., Mazzarella, J. M. & Uomoto, A. 1989, ApJ, 342, 364.Google Scholar
MacAlpine, G. M., Lawrence, S. S., Uomoto, A., Lowenthal, J. D., Woodgate, B. E., Brown, L. W., & Oliversen, R. J. 1993, ApJ, 432, L131 Google Scholar
Michel, F. C, Scowen, P. A., Dufour, R. J. & Hester, J. J. 1991, ApJ, 368, 363.Google Scholar
Pequignot, D. & Dennefeld, M. 1983, A&A, 120, 249.Google Scholar
Stone, J. M. & Norman, M. L. 1992, ApJ, 390, L17.Google Scholar
Uomoto, A. & MacAlpine, G. M. 1987, AJ, 93 1511.Google Scholar
Wu, C.-C., Crenshaw, D. M., Fesen, R. A., Hamilton, A. J. S. & Sarazin, C. L. 1993, ApJ, 416, 247.Google Scholar