- Abstract:
-
We present optical monitoring of the black hole candidate XTE J1752-223 during its 2009-10 outburst and decay to quiescence. The optical light curve can be described by an exponential decay followed by a plateau, then a more rapid fade towards quiescence. The plateau appears to be due to an extra component of optical emission that brightens and then fades over ∼40days. We show evidence for the origin of this optical 'flare' to be the synchrotron jet during the decaying hard state, and we iden...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2011.19839.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 419
- Issue:
- 2
- Pages:
- 1740-1751
- Publication date:
- 2012-01-05
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:3adc03f7-382c-4555-9e36-f88a7276f094
- Source identifiers:
-
361969
- Local pid:
- pubs:361969
- Language:
- English
- Keywords:
- Copyright date:
- 2012
Journal article
A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223
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