Identification of the Low-Mass X-Ray Binary and Faint X-Ray Sources in NGC 6652
Powerful CMD: a tool for color-magnitude diagram studies
Surface Brightness Profiles of Galactic Globular Clusters from Hubble Space Telescope Images
Testing Photometric Diagnostics for the Dynamical State and Possible Intermediate-mass Black Hole Presence in Globular Clusters
The ACS survey of Galactic globular clusters. XII. Photometric binaries along the main sequence
The Age of the Inner Halo Globular Cluster NGC 6652
Ultracompact X-Ray Binaries in Globular Clusters: Variability of the Optical Counterpart of X1832-330 in NGC 6652
Using binaries in globular clusters to catch sight of intermediate-mass black holes
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-09-05T07:30:13Z/1997-09-05T11:24:53Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Chaboyer comma Brian, 1998, 'The Formation of the Inner Galactic Halo', 1.0, European Space Agency, https://doi.org/10.5270/esa-o67l561