Radio afterglow of the jetted tidal disruption event Swift J1644+57
The recent transient event Swift J1644+57 has been interpreted as resulting from a relativistic outflow, powered by the accretion of a tidally disrupted star onto a supermassive black hole. This discovery of a new class of relativistic transients opens new windows into the study of tidal disruption...
Main Authors: | Mimica P., Giannios D., Metzger B.D. |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2012-12-01
|
Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20123904001 |
Similar Items
-
The first months in the lifetime of the newly born jet associated to Swift J1644+57
by: Pérez-Ramírez D., et al.
Published: (2012-12-01) -
The first two years in the lifetime of the newly born jet associated to Sw J1644+57
by: Castro-Tirado A. J., et al.
Published: (2013-12-01) -
Beam profile indicator for swift heavy ions using phosphor afterglow
by: T. Z. Zhan, et al.
Published: (2012-09-01) -
Numerical study of emission and dynamics from a TDE-powered jet
by: Metzger B., et al.
Published: (2012-12-01) -
Radio follow-up observations of stellar tidal disruption flares: Constraints on off-axis jets
by: Körding E., et al.
Published: (2012-12-01)