Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.8404e&link_type=abstract
American Astronomical Society, 197th AAS Meeting, #84.04; Bulletin of the American Astronomical Society, Vol. 32, p.1547
Astronomy and Astrophysics
Astronomy
Scientific paper
The globular cluster 47 Tuc is ideal for studies of cluster binaries because of its proximity, large mass and diverse range of binary species. We report the use of superb quality Chandra and HST imaging to make optical identifications of X-ray sources in and around the dense core of this cluster. The detailed X-ray results will be described in a separate paper by Grindlay et al. The optical imaging is the deepest ever obtained of this beautiful cluster, involving intensive 8.3 day V/I observations with HST/WFPC2. These observations were optimized for variability work and reach unprecedented sensitivity, with rms noise levels of ~4 mmag per exposure near the main sequence turnoff (and ~650 exposures in each of V and I). Supplementary F336W observations provide good color information. The Chandra images are exquisite, delivering the expected dramatic improvement over ROSAT images and containing over 100 sources within 1' of the cluster center. The positional errors for the brighter Chandra sources are a few tenths of an arcsecond, allowing, for the first time, unambiguous optical identifications. This work is ongoing, but already large numbers of X-ray sources have been identified, including cataclysmic variables, eclipsing binaries and possible low-mass X-ray binaries. Also, interesting limits have been set for X-ray sources (possibly millisecond pulsars) not associated with optically variable stars. This work is partially supported by HST grant GO-8267.
Albrow Michael D.
Edmonds Peter D.
Gilliland Ron L.
Grindlay Jonathon E.
Guhathakurta Puraga
No associations
LandOfFree
HST Optical Studies of Chandra X-ray Sources in 47 Tucanae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with HST Optical Studies of Chandra X-ray Sources in 47 Tucanae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HST Optical Studies of Chandra X-ray Sources in 47 Tucanae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1726790