Afterglow model for the radio emission from the jetted tidal disruption candidate Swift J1644+57
出版年份 2012 全文链接
标题
Afterglow model for the radio emission from the jetted tidal disruption candidate Swift J1644+57
作者
关键词
-
出版物
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume -, Issue -, Pages no-no
出版商
Oxford University Press (OUP)
发表日期
2012-01-18
DOI
10.1111/j.1365-2966.2011.20273.x
参考文献
相关参考文献
注意:仅列出部分参考文献,下载原文获取全部文献信息。- X-RAY AND RADIO CONSTRAINTS ON THE MASS OF THE BLACK HOLE IN SWIFT J164449.3+573451
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- BLACK HOLE SPIN IN Sw J1644+57 and Sw J2058+05
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- (2011) Geoffrey C. Bower Astrophysical Journal Letters
- RELATIVISTIC JET DYNAMICS AND CALORIMETRY OF GAMMA-RAY BURSTS
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- Radio transients from stellar tidal disruption by massive black holes
- (2011) Dimitrios Giannios et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Relativistic jet activity from the tidal disruption of a star by a massive black hole
- (2011) D. N. Burrows et al. NATURE
- Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451
- (2011) B. A. Zauderer et al. NATURE
- An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
- (2011) A. J. Levan et al. SCIENCE
- A Possible Relativistic Jetted Outburst from a Massive Black Hole Fed by a Tidally Disrupted Star
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- Multiband light curves of tidal disruption events
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- Jet opening angles and gamma-ray brightness of AGN
- (2009) A. B. Pushkarev et al. ASTRONOMY & ASTROPHYSICS
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- (2009) Suvi Gezari et al. ASTROPHYSICAL JOURNAL
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- (2009) Weiqun Zhang et al. ASTROPHYSICAL JOURNAL
- Optical flares from the tidal disruption of stars by massive black holes
- (2009) Linda E. Strubbe et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Deceleration of arbitrarily magnetized GRB ejecta: the complete evolution
- (2008) P. Mimica et al. ASTRONOMY & ASTROPHYSICS
- UV/Optical Detections of Candidate Tidal Disruption Events byGALEXand CFHTLS
- (2008) S. Gezari et al. ASTROPHYSICAL JOURNAL
- Stellar disruption by a supermassive black hole: is the light curve really proportional tot−5/3?
- (2008) G. Lodato et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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