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Gamma-Ray Imaging of the Galactic Center Region

  • W. R. Cook
  • D. M. Palmer
  • T. A. Prince
  • S. M. Schindler
  • C. H. Starr
  • E. C. Stone
Conference paper
Part of the International Astronomical Union Union Astronomique Internationale book series (IAUS, volume 136)

Abstract

The Caltech imaging γ-ray telescope was launched by balloon from Alice Springs, NT, Australia and performed observations of the galactic center during the period 12.62 to 13.00 April 1988 UT. The first coded-aperture images of the galactic center region at energies above 30 keV show a single strong γ-ray source which is located 0.7±0.1 ° from the galactic nucleus and is tentatively identified as 1E1740.7-2942. If the source is at the distance of the galactic center, it is one of the most luminous objects in the galaxy at energies from 35 to 200 keV.

Keywords

Galactic Center Crab Nebula Star Camera Luminous Object Galactic Center Region 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. (1).
    Leventhal, M. 1987, in 13th Texas Symposium on Relativistic Astrophysics, edited by M. Ulmer, 382.Google Scholar
  2. (2).
    Lingenfelter, R. E., and Ramaty, R. 1988, review in these proceedings.Google Scholar
  3. (3).
    Skinner, G. K., review in these proceedings.Google Scholar
  4. (4).
    Matteson, J. L. 1982, in The Galactic Center, edited by G. R. Riegler and R. D. Blandford, AIP Conf. Proc. No. 83, 109.Google Scholar
  5. (5).
    Skinner, G. K. et al. 1987, Nature, 330, 544.ADSCrossRefGoogle Scholar
  6. (6).
    Kawai, N. et al. 1988, Ap. J., 330, 130.ADSCrossRefGoogle Scholar
  7. (7).
    Watson, M. G., Willingale, R., Grindlay, J. E., and Hertz, P. 1981, Ap. J., 250, 142.ADSCrossRefGoogle Scholar
  8. (8).
    Leventhal, M., MacCallum, C. J., Huters, A. F., and Stang, P. D. 1982, Ap. J., 260, L1.ADSCrossRefGoogle Scholar
  9. (9).
    Riegler, G. R. et al. 1981, Ap. J., 248, L13.ADSCrossRefGoogle Scholar
  10. (10).
    Riegler, G. R. et al. 1985, Ap. J., 294, L13.ADSCrossRefGoogle Scholar
  11. (11).
    Althouse, W. E. et al. 1985, Proc. 19th Int. Cosmic Ray Conf. (La Jolla), 3, 299.Google Scholar
  12. (12).
    Levine, A. M. et al. 1984, Ap. J. Suppl., 54, 581.ADSCrossRefGoogle Scholar
  13. (13).
    Jung, G. V. 1986, Ph.D. thesis, University of California at San Diego.Google Scholar
  14. (14).
    Ling, J. C., Mahoney, W. A., Wheaton, Wm. A., and Jacobson, A. S. 1987, Ap. J., 321, L117.ADSCrossRefGoogle Scholar
  15. (15).
    Skinner, G. K., poster paper this conference.Google Scholar
  16. (16).
    Knight, K. F., Johnson III W. N., Kurfess, J. D., and Strickman, M. S. 1985, Ap. J., 290, 557.ADSCrossRefGoogle Scholar
  17. (17).
    Dennis, B. R. et al. 1980, Ap. J., 236, L49.ADSCrossRefGoogle Scholar

Copyright information

© IAU 1989

Authors and Affiliations

  • W. R. Cook
    • 1
  • D. M. Palmer
    • 1
  • T. A. Prince
    • 1
  • S. M. Schindler
    • 1
  • C. H. Starr
    • 1
  • E. C. Stone
    • 1
  1. 1.California Institute of TechnologyPasadenaUSA

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