Mechanism of very high-energy radiation in BL Lacertae object 3C 66A
Mechanism of very high-energy radiation in BL Lacertae object 3C 66A
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BL 蜥蜴天体 3C 66A 中极高能辐射的机制
DOI：
10.1051/0004-6361/200913035
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发表时间：
2009-11
影响因子：
6.5
通讯作者：
Wang, Jiancheng
中科院分区：
文献类型：
--
作者：
Yang, Jianping;Wang, Jiancheng
目标。我们的目标是了解耀变体的性质和产生高能的机制。射线，通过调查blazar 3C 66A。方法.我们模拟了最近用Fermi-LAT和VERITAS望远镜观测到的3C 66A的高能光谱。在两台望远镜最近几乎同时观测到的能量范围从0.2 - 100 GeV到200 - 500 GeV的光谱有一个很难的变化。结果去吸收的VERITAS光谱强烈依赖于红移，这是高度不确定的。如果采用z = 0.444，我们可以使用SSC模型来产生Fermi-LAT分量，使用EC模型来产生VERITAS分量。然而，如果z = 0.1，则本征VERITAS光谱将更柔和，并且可以使用SSC模型解释费米LAT和VERITAS光谱之间的平滑链接。
Aims. Our goal is to understand the nature of blazars and the mechanisms for generating high-energy.-rays, through investigation of the blazar 3C 66A. Methods. We model the high-energy spectrum of 3C 66A, which was observed recently with the Fermi-LAT and VERITAS telescopes. The spectrum has a hard change from the energy range of 0.2-100 GeV to 200-500 GeV in recent almost contemporaneous observations of two telescopes. Results. The de-absorbed VERITAS spectrum depends strongly on redshift, which is highly uncertain. If z = 0.444 is adopted, we are able to use the SSC model to produce the Fermi-LAT component and the EC model to the VERITAS component. However, if z = 0.1, the intrinsic VERITAS spectrum will be softer, and there will be a smooth link between the Fermi-LAT and VERITAS spectra that can be explained using an SSC model.
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DOI：
10.1086/533521
发表时间：
2008-01
期刊：
The Astrophysical Journal
影响因子：
--
作者：
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通讯作者：
B. Piner;Niraj Pant;Philip G. Edwards
DOI：
10.1086/320858
发表时间：
2001-01
期刊：
The Astrophysical Journal Supplement Series
影响因子：
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作者：
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通讯作者：
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DOI：
10.1051/0004-6361:20078492
发表时间：
2007-11
期刊：
arXiv: Astrophysics
影响因子：
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作者：
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通讯作者：
J. Finke;J. Shields;M. Boettcher;S. Basu
DOI：
10.1086/173251
发表时间：
1993-10
期刊：
The Astrophysical Journal
影响因子：
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作者：
C. Dermer;R. Schlickeiser
通讯作者：
C. Dermer;R. Schlickeiser
DOI：
10.1086/592244
发表时间：
2008-08
期刊：
The Astrophysical Journal Letters
影响因子：
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作者：
V. C. V. Acciari-V.-C.-V.-Acciari-2077280781;E. Aliu;M. Beilicke;W. Benbow;M. Boettcher;S. Bradbury;J. Buckley;V. Bugaev;Y. Butt;O. Celik;A. Cesarini;L. Ciupik;Y. Chow;P. Cogan;P. Colin;W. Cui;M. Daniel;T. Ergin;A. Falcone;S. Fegan;J. Finley;G. Finnegan;P. Fortin;L. Fortson;A. Furniss;D. Gall;G. Gillanders;J. Grube;R. Guenette;G. Gyuk;D. Hanna;E. Hays;J. Holder;D. Horan;C. Hui;T. Humensky;A. Imran;P. Kaaret;N. Karlsson;M. Kertzman;D. Kieda;A. Konopelko;H. Krawczynski;F. Krennrich;M. Lang;S. LeBohec;K. Lee;G. Maier;A. McCann;M. McCutcheon;P. Moriarty;R. Mukherjee;T. Nagai;J. Niemiec;R. Ong;D. Pandel;J. Perkins;D. Petry;M. Pohl;J. Quinn;K. Ragan;L. Reyes;P. Reynolds;E. Roache;H. Rose;M. Schroedter;G. Sembroski;A. Smith;D. Steele;S. Swordy;J. Toner;V. Vassiliev;R. Wagner;S. Wakely;J. Ward;T. Weekes;A. Weinstein;R. White;D. Williams;S. Wissel;M. Wood;B. Zitzer
通讯作者：
V. C. V. Acciari-V.-C.-V.-Acciari-2077280781;E. Aliu;M. Beilicke;W. Benbow;M. Boettcher;S. Bradbury;J. Buckley;V. Bugaev;Y. Butt;O. Celik;A. Cesarini;L. Ciupik;Y. Chow;P. Cogan;P. Colin;W. Cui;M. Daniel;T. Ergin;A. Falcone;S. Fegan;J. Finley;G. Finnegan;P. Fortin;L. Fortson;A. Furniss;D. Gall;G. Gillanders;J. Grube;R. Guenette;G. Gyuk;D. Hanna;E. Hays;J. Holder;D. Horan;C. Hui;T. Humensky;A. Imran;P. Kaaret;N. Karlsson;M. Kertzman;D. Kieda;A. Konopelko;H. Krawczynski;F. Krennrich;M. Lang;S. LeBohec;K. Lee;G. Maier;A. McCann;M. McCutcheon;P. Moriarty;R. Mukherjee;T. Nagai;J. Niemiec;R. Ong;D. Pandel;J. Perkins;D. Petry;M. Pohl;J. Quinn;K. Ragan;L. Reyes;P. Reynolds;E. Roache;H. Rose;M. Schroedter;G. Sembroski;A. Smith;D. Steele;S. Swordy;J. Toner;V. Vassiliev;R. Wagner;S. Wakely;J. Ward;T. Weekes;A. Weinstein;R. White;D. Williams;S. Wissel;M. Wood;B. Zitzer