C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: The tidal disruption of a star by a black hole provides a unique opportunity to study accretion physics. Recently, delayed radio flares have been discovered in several TDEs, peaking years after their optical emission has faded. Various explanations have been proposed, including off-axis jets entering our line of sight, delayed accretion disk formation, or a state change in the accretion flow. To elucidate the origin(s) of these flares, it has become crucial to acquire radio and X-ray observations of these events at late-times (~ months to years post-discovery) to study this previously unexplored phase in the lifetime of TDEs. |
Remarks: We require co-ordinated follow-up of X-rays and radio with the VLA (within 30 days of the Chandra observations), however we do not need the X-ray observations to be planned in any one particular time window during Cycle 24. |
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