BATSE All-Sky Search for Transient Gamma-Ray Lines between 300 and 550 keV
暂无分享,去创建一个
[1] Gerald J. Fishman,et al. All-Sky Search for Transient Sources Near 0.5 MeV with the Burst and Transient Source Experiment (BATSE) , 1996 .
[2] J. Bally,et al. Is the Galactic Centre gamma-ray source 1E1740.7 – 2942 accreting from a molecular cloud? , 1991, Nature.
[3] M. Niel,et al. DETECTION OF A FEATURE AT 0.44 MEV IN THE CRAB PULSAR SPECTRUM WITH FIGARO-II - A REDSHIFTED POSITRON-ANNIHILATION LINE , 1991 .
[4] H. Murakami,et al. A Balloon Investigation of Galactic ?-ray Lines with a High Resolution Ge(Li) Spectrometer , 1979 .
[5] C. A. Ayre,et al. Gamma-ray line features from the Crab Nebula in the energy range 50–2000 keV , 1983 .
[6] N. Khavenson,et al. X-ray nova in Musca (GRS 1124 - 68) - Hard X-ray source with narrow annihilation line , 1992 .
[7] M. Leventhal,et al. A search for gamma-ray lines from Nova Cygni 1975, Nova Serpentis 1970, and the Crab Nebula , 1977 .
[8] R. Misra,et al. Formation of a Jet in the Galactic Center Black Hole Candidate 1E 1740.7-2942 , 1993 .
[9] R. Ramaty,et al. On the origin of variable 511 keV line emission from the Galactic center region , 1992 .
[10] M. Livio,et al. The Dual Nature of Hard X-Ray Outbursts from the Superluminal X-Ray Transient Source GRO J1655–40 , 1996, astro-ph/9610212.
[11] P. Durouchoux,et al. Gamma-ray line astrophysics , 1991 .
[12] N. Khavenson,et al. SIGMA/GRANAT soft gamma-ray observations of the X-ray nova in Musca : discovery of positron annihilation emission line , 1992 .
[13] E. Costa,et al. Observation of the Crab pulsar, PSR 0531 + 21, at 0. 2-6. 0 MeV with the Figaro II experiment , 1990 .