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EUV Observations of Pulsars

Published online by Cambridge University Press:  12 April 2016

Jerry Edelstein  and
Stuart Bowyer
Jerry Edelstein
Affiliation:
Center for EUV Astrophysics University of California 2150 Kittredge Street Berkeley, CA 94720-5030, USA
Stuart Bowyer
Affiliation:
Center for EUV Astrophysics University of California 2150 Kittredge Street Berkeley, CA 94720-5030, USA

Abstract

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Three pulsars have been detected with the Lexan (100 Å )filter of the EUVE Deep Survey telescope: the middle-aged isolated pulsars, PSR B0656+14 and Geminga, plus the aged millisecond pulsar PSR J0437–4715. The EUV detections have been used both alone and in combination with observations in other bandpasses to limit the physical state of the objects and to test theories regarding neutron star cooling and re-heating mechanisms. For Geminga, the EUVE data suggests the presence of an optical cyclotron spectral feature superimposed on the Rayleigh-Jeans continuum tail from a hot pulsar surface. We summarize EUV pulsar observations and results.

Information

Type
Part 5 High Energy Phenomena
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 291 - 295
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Arons, J. & Tavani, M. 1993, ApJ, 403, 249 Google Scholar
Becker, W. & Trumper, J. 1993, Nature, 365, 528 Google Scholar
Bignami, G.F, Caraveo, P.A, Mignani, R., Edelstein, J., and Bowyer, S. 1996, ApJ, 456, L111 CrossRefGoogle Scholar
Bignami, G.F., Caraveo, P.A. and Paul, J.A. 1988 å, 202, L1 Google Scholar
Caraveo, P.A., Bignami, G.F., Mereghetti, S. 1994 ApJ, 422, L87 CrossRefGoogle Scholar
Cordova, F.A. et al. ApJ, 1989, 345, 451 CrossRefGoogle Scholar
Edelstein, J., Foster, R.S., & Bowyer, S. 1995, ApJ, 454, 442 Google Scholar
Finley, J.P, Ogelman, H., & Kiziloglu, U 1992, ApJ, 394, L21 CrossRefGoogle Scholar
Finley, J.P., Ogelman, H., & Edelstein, J 1994, BAAS, 26, 870 Google Scholar
Foster, R.S., Edelstein, J. & Bowyer, S. 1996, ”Astrophysics in the EUV”, Kluwer, Dortrecht Google Scholar
Foster, R.S. 1995, private communicationGoogle Scholar
Freese, K., Turner, M., & Schramm, D.N. 1983, Phys.Rev.Lett, 51, 1625 Google Scholar
Fruscione, A., Hawkins, I., Jelinsky, P., & Wiercigroch, A., 1994, ApJS, 94, 127 CrossRefGoogle Scholar
Halpern, J.P. and Ruderman, M. 1993, ApJ, 415, 286 CrossRefGoogle Scholar
Halpern, J.P. and Tytler, D. 1988, ApJ, 330, 201 Google Scholar
Haplern, J.P, Marshall, H.M and Martin, D.C, submitted, 1996.Google Scholar
Kolb, E. & Turner, M. 1984, ApJ, 286, 702 CrossRefGoogle Scholar
Possenti, A., Mereghetti, S. & Colpi, M. 1996, A&A, in press.Google Scholar
Shibazaki, N. & Lamb, F.K. 1989, ApJ, 346, 808 CrossRefGoogle Scholar
Taylor, J.H., Manchester, R.N. & Lyne, A.G. 1993, ApJS, 88, 529 CrossRefGoogle Scholar