The New Gamma‐Ray Astronomy

作者: Neil Gehrels , Jacques Paul

DOI: 10.1063/1.882139

关键词:

摘要: Our understanding of the gamma‐ray sky is being revolutionized. Seven years ago, astronomers knew only a scattering very bright sources. Now, thanks to two international observatories, appears be teeming with variety—unstable sources that change violently on short time scales, steady glow radioactively and others whose nature we barely understand.

参考文章(8)
M. J. REES, New interpretation of extragalactic radio sources. Nature. ,vol. 229, pp. 312- 317 ,(1971) , 10.1038/229312A0
I. F. Mirabel, L. F. Rodríguez, B. Cordier, J. Paul, F. Lebrun, A double-sided radio jet from the compact Galactic Centre annihilator 1E1740.7-2942 Nature. ,vol. 358, pp. 215- 217 ,(1992) , 10.1038/358215A0
E. E. Salpeter, Accretion of Interstellar Matter by Massive Objects. The Astrophysical Journal. ,vol. 140, pp. 796- 800 ,(1964) , 10.1086/147973
E. Margaret Burbidge, G. R. Burbidge, William A. Fowler, F. Hoyle, Synthesis of the Elements in Stars Reviews of Modern Physics. ,vol. 29, pp. 547- 650 ,(1957) , 10.1103/REVMODPHYS.29.547
D. LYNDEN-BELL, GALACTIC NUCLEI AS COLLAPSED OLD QUASARS. Nature. ,vol. 223, pp. 690- 694 ,(1969) , 10.1038/223690A0
Wan Chen, Wan Chen, Wei Cui, S. N. Zhang, S. N. Zhang, Black Hole Spin in X-Ray Binaries: Observational Consequences The Astrophysical Journal. ,vol. 482, ,(1997) , 10.1086/310705
S. N. Zhang, Wei Cui, Wan Chen, Black Hole Spin in X-Ray Binaries: Observational Consequences The Astrophysical Journal. ,vol. 482, pp. L155- L158 ,(1997) , 10.1086/310705