Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Shan–qun Zhan"'
Publikováno v:
Chinese Astronomy and Astrophysics. 18:54-59
We assume that the soft gamma-ray repeater GB 790107 comes from a weakly magnetized ( B ∼ 10 8 G) neutron star, where shower-type accretion of cometary material results in an optically thick region on the surface of the star. The temperature distri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::52dd2f57a1b940a5b1145e1ba4804672
https://doi.org/10.1016/0275-1062(94)90070-1
https://doi.org/10.1016/0275-1062(94)90070-1
Autor:
Shan-qun Zhan, Tian-yi Shi
Publikováno v:
Chinese Astronomy and Astrophysics. 17:26-32
When radiation loss is considered, we believe that synchrotron radiation of particles beamed along magnetic field generated by such acceleration mechanism as field reconnection is the main mechanism for producing gamma-ray bursts. On the basis of thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::de4053a225cce4c22a047487dda5c3c5
https://doi.org/10.1016/0275-1062(93)90037-p
https://doi.org/10.1016/0275-1062(93)90037-p
Autor:
Shan–qun Zhan, Tian–yi Shi
Publikováno v:
Communications in Theoretical Physics. 14:333-344
A model of the old and hot neutron stars (age , temperature ) with the low magnetic field as the sources of Gamma-ray bursts is presented. In the range of medium energy , the main radiation mechanism is still the thermal synchrotron radiation. The ab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dbfd84bf43719c04a9232e68a7896b21
https://doi.org/10.1088/0253-6102/14/3/333
https://doi.org/10.1088/0253-6102/14/3/333