Ages for Globular Clusters in the Outer Galactic Halo: The Second-Parameter Clusters Palomar 3, Palomar 4, and Eridanus
Horizontal-Branch Models and the Second-Parameter Effect. IV. The Case of M3 and Palomar 3
The Central Blue Straggler Population in Four Outer-halo Globular Clusters
The velocity dispersion and mass function of the outer halo globular cluster Palomar 4
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-04-12T21:27:17Z/1995-04-19T18:00:46Z
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, Hesser comma James E., 1996, 'AGES FOR THE OUTERMOST GLOBULAR CLUSTERS: THE FORMATION OF THE GALACTIC HALO: CYCLE 4 HIGH, PART II', 1.0, European Space Agency, https://doi.org/10.5270/esa-b6bu7iz