首页 | 本学科首页   官方微博 | 高级检索  
     检索      

Simultaneous Multi-Wavelength Observations of the TeV Blazar Mrk 421 during February - March, 2003: X-Ray and NIR Correlated Variability
作者单位:[1]Center for Astrophysics, Guangzhou University, Guangzhou 510006, China [2]Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai - 400 005, India [3]Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital - 263129,India
基金项目:国家自然科学基金,国家重点基础研究发展计划(973计划)
摘    要:

关 键 词:丙烯腈  X射线  变异性  耀变体  观察报告

Simultaneous Multi-Wavelength Observations of the TeV Blazar Mrk 421 during February - March, 2003: X-Ray and NIR Correlated Variability
Authors:Alok C Gupta B S Acharya Debanjan Bose Varsha R Chitnis Jun-Hui Fan
Abstract:We report the result of simultaneous multi-wavelength observations of the TeV blazar Mrk 421 during February - March 2003. We observed Mrk 421 using the Pachmarhi Array of Cerenkov Telescopes (PACT) of Tata Institute of Fundamental Research at Pachmarhi, India. Other simultaneous data were taken from the literature and public data archives. We have analyzed the high quality X-ray (2-20keV) observations from the NASA Rossi X-Ray Timing Explorer (RXTE). We obtained a possible correlated variability between X-ray and J band (1.25 μ) near infrared (NIR) wavelength. This is the first case of X-ray and NIR correlated variability in Mrk 421 or any high energy peaked (HBL) blazar. The correlated variability reported here indicates a similar origin for the NIR and X-ray emissions. The emission is not affected much by the environment of the surrounding medium of the central engine of Mrk 421. The observations are consistent with the shock-in-jet model for the emissions.
Keywords:galaxies: active - galaxies: blazars: general - galaxies: blazars: individual: Mrk 421
本文献已被 维普 万方数据 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号