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THE OPTICAL COUNTERPART TO THE X-RAY TRANSIENT IGR J1824–24525 IN THE GLOBULAR CLUSTER M28.
- Source :
- Astrophysical Journal; 8/20/2013, Vol. 773 Issue 2, p1-6, 6p
- Publication Year :
- 2013
-
Abstract
- We report on the identification of the optical counterpart to the recently detected INTEGRAL transient IGR J1824–24525 in the Galactic globular cluster M28. From analysis of a multi-epoch Hubble Space Telescope data set, we have identified a strongly variable star positionally coincident with the radio and Chandra X-ray sources associated with the INTEGRAL transient. The star has been detected during both a quiescent and an outburst state. In the former case it appears as a faint, unperturbed main-sequence star, while in the latter state it is about two magnitudes brighter and slightly bluer than main-sequence stars. We also detected Ha excess during the outburst state, suggestive of active accretion processes by the neutron star. [ABSTRACT FROM AUTHOR]
- Subjects :
- X-ray research
GLOBULAR clusters
NEUTRONS
Subjects
Details
- Language :
- English
- ISSN :
- 0004637X
- Volume :
- 773
- Issue :
- 2
- Database :
- Complementary Index
- Journal :
- Astrophysical Journal
- Publication Type :
- Academic Journal
- Accession number :
- 90179289
- Full Text :
- https://doi.org/10.1088/0004-637X/773/2/122