Optical identification of X- and gamma-ray sources: the use of existing data-Reference-Cited by-同舟云学术

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Optical identification of X- and gamma-ray sources: the use of existing data

Published:1992-09 Issue:5 Volume:15 Page:899-903
ISSN:0390-5551
Container-title:Il Nuovo Cimento C
language:en
Short-container-title:Il Nuovo Cimento C

Author:

Pizzichini G.,Cristallo M. R.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.1007/BF02507864.pdf

Reference22 articles.

1. J. P. Halpern andD. Tytler:Astrophys. J.,330, 201 (1988).

2. T. L. Cline, U. D. Desai, B. J. Teegarden, W. D. Evans, R. W. Klebesadel, J. G. Laros, C. Barat, K. Hurley, M. Niel, G. Vedrenne, I. V. Estulin, V. G. Kurt, G. A. Mersov, V. M. Zenchenko, M. C. Weisskopf andJ. Grindlay:Astrophys. J.,255, L45 (1982).

3. H. Pedersen, G. Pizzichini, B. Schaefer andK. Hurley:Gamma-Ray Bursts, Proceedings of the AIPConference No. 141, edited by.E. P. Liang andV. Petrosian (AIP Press, New York, 1986), p. 39.

4. M. Boer, K. Hurley, M. Gottardi, C. Motch, H. Pedersen andR. L. Simonsen:Astron. Astrophys.,214, 148 (1989).

5. G. Pizzichini:Conference Papers, XXI ICRC,Adelaide, Vol.1, (1990), p. 53.

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