Gamma-ray emission from pulsar/massive-star binaries

被引：0
作者：
Romero, Gustavo E. [1 ]
机构：
[1] Consejo Nacl Invest Cient & Tecn, IAR, CCT La Plata, RA-1033 Buenos Aires, DF, Argentina
来源：
HIGHLIGHTS OF ASTRONOMY, VOL 15 | 2010年 / 15卷
关键词：
Radiation mechanisms: non-thermal; stars: neutron; stars: early-type; stars: winds; outflows; gamma rays: observations; gamma rays: theory; X-RAY; MICROQUASAR LS-I+61-303; LS-5039; DISCOVERY; PERIASTRON; RADIATION; ACCRETION; RADIO; HESS;
D O I：
10.1017/S1743921310008501
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I present a review of the main phenomenological properties at high energies related to massive gamma-ray binaries and I discuss some aspects of pulsar models for these objects.
引用
收藏
页码：126 / 130
页数：5
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