首页> 外文OA文献 >Extremely rapid bursts of TeV photons from the active galaxy Markarian 421
【2h】

Extremely rapid bursts of TeV photons from the active galaxy Markarian 421

机译:来自活跃的星系标记421的Tev Photons非常快速

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。
获取外文期刊封面目录资料

摘要

DISCRETE astronomical sources of photons in the TeV energy range are believed to be associated with regions in the relativistic outflow of particles and radiation from compact objects, such as neutron stars and black holes. The Bur from such sources, together with the timescales on which they vary, can provide strong constraints on the emission mechanisms. Here we report the observation of two dramatic outbursts of TeV photons from the active galaxy Markarian 421 (Mrk421). In the first outburst, which had a doubling time of about one hour, the flux increased above the relatively quiescent value by more than a factor of 50, briefly making Mrk421 the brightest TeV source in the sky. In the second outburst, which lasted approximately 30 minutes, the flux increased by a factor of 20-25. These data suggest that the emission region is extremely small-perhaps even smaller than our Solar System. This could prove challenging for current theoretical models of such emissions.
机译:TEV能量范围中的离散天文源的光子被认为与颗粒的相对论流出的区域相关联,以及来自紧凑型物体的辐射,例如中子恒星和黑洞。来自这些来源的BUS与它们变化的时间表一起,可以为排放机制提供强大的限制。在这里,我们举报了从活性星系标记421(MRK421)的两个戏剧性的Tev光子爆发的观察。在第一次爆发中,在大约一个小时的倍增时间下,磁通量高于相对静止的值,超过50倍,简要制作MRK421在天空中最亮的TEV源。在持续大约30分钟的第二次爆发中,通量增加了20-25倍。这些数据表明,排放区域非常小 - 甚至可能比我们的太阳系小。这可能证明对这种排放的当前理论模型有挑战性。

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号