A far-ultraviolet variable with an 18-minute period in the globular cluster NGC 1851
An Ultraviolet-Excess Optical Candidate for the Luminous Globular Cluster X-Ray Source in NGC 1851
Central dynamics of globular clusters
Far-Ultraviolet Observations of RR Lyrae Stars in the Core of NGC 1851
Hubble Space Telescope Reveals Multiple Sub-giant Branch in Eight Globular Clusters
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. III. The Double Subgiant Branch of NGC 1851
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-04-10T06:23:16Z/1996-04-10T09:47:16Z
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, Bohlin comma Ralph C., 1997, 'GLOBULAR CLUSTER CORE STRUCTURE AND DYNAMICS (FOS 36) - CYCLE 4 CARRYOVER', 1.0, European Space Agency, https://doi.org/10.5270/esa-rrrbu53