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X-ray Studies of SS433

Published online by Cambridge University Press:  04 August 2017

J. E. Grindlay ,
D. Band ,
F. Seward ,
L. Stella  and
M. Watson
J. E. Grindlay
Affiliation:
Smithsonian/Harvard Center for Astrophysics
D. Band
Affiliation:
Smithsonian/Harvard Center for Astrophysics
F. Seward
Affiliation:
Smithsonian/Harvard Center for Astrophysics
L. Stella
Affiliation:
Smithsonian/Harvard Center for Astrophysics
M. Watson
Affiliation:
University of Leicester

Extract

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Results of Einstein Observations of SS433 are discussed which address both the nature of the diffuse X-ray lobes and the relationships between SS433 and W50 as well as the time variability and nature of the central X-ray source. The diffuse X-ray lobes extend out to the quasi-spherical shell seen in the radio maps of W50 and suggest that the X-ray lobes are powered by the interaction of shock-heating from the SS433 jets and the denser material in the W50 shell. The central X-ray source in SS433 is time variable but only on timescales ≳ 500–1000 sec. Flares, in which the non-thermal spectrum hardens, are detected at two preferred phases in the 13.08 day binary orbit. Constraints on the central X-ray source size as well as a possible eclipse by the companion star suggest the compact object in SS433 may be an ~10 M⊙ black hole.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 459 - 463
Copyright
Copyright © Reidel 1983 

References

Avni, Y. and Schiller, N. 1982, Ap. J., 257, 703.Google Scholar
Crampton, D. and Hutchings, J. 1981, Ap. J., 251, 604.Google Scholar
Giacconi, R., et al. 1979, Ap. J., 230, 540.Google Scholar
Grindlay, J., Band, D., Seward, F., Leahy, D., Weisskopf, M., and Marshall, F. 1983, Ap. J., submitted.Google Scholar
Margon, B. 1982, Science, 215, 247.Google Scholar
Papaloizou, J. and Pringle, J.E. 1982, MNRAS, 200, 49.Google Scholar
Seaquist, E., Gilmore, W., Johnston, K., and Grindlay, J. 1982, Ap. J., 260, 220.Google Scholar
Seward, F., Page, C., Turner, M., and Pounds, K. 1976, MNRAS, 175, 39.CrossRefGoogle Scholar
Seward, F., Grindlay, J., Seaquist, E., and Gilmore, W. 1980, Nature, 287, 806.Google Scholar
Watson, M., Willingale, R., Grindlay, J., and Seward, F. 1983, Ap. J., submitted.Google Scholar
Zealey, W., Dopita, M., and Martin, D.F. 1980, MNRAS, 192, 731.CrossRefGoogle Scholar