A Spectroscopic Analysis of Blue Stragglers, Horizontal Branch Stars, and Turnoff Stars in Four Globular Clusters
Blue Straggler Stars: A Direct Comparison of Star Counts and Population Ratios in Six Galactic Globular Clusters
HST observations of blue Straggler stars in the core of the globular cluster M 3.
HST/WFPC2 observation of the core of M 3: Blue objects and the position of the radio source
Hubble Space Telescope Discovery of an Optical Counterpart to the Supersoft X-Ray Source in the Globular Cluster M3
Hubble Space Telescope Ultraviolet Observations of the Cores of M3 and M13
On the Globular Cluster Initial Mass Function below 1 Msolar
The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions
The Chemical Composition Contrast between M3 and M13 Revisited: New Abundances for 28 Giant Stars in M3
The Distribution of Collisionally Induced Blue Stragglers in the Color-Magnitude Diagram
The lower main sequence of the globular cluster M3 with the Hubble Space Telescope: luminosity and mass functions
The Luminosity Function of M3
The RR Lyrae star period - K-band luminosity relation of the globular cluster M 3
The stellar population of the globular cluster M 3. II. CCD photometry of additional 10,000 stars.
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-04-25T10:17:16Z/1995-04-25T21:52:17Z
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, Fusi Pecci comma Flavio, 1996, 'M3: AN IDEAL LABORATORY FOR TESTING STELLAR EVOLUTION AND DYNAMICS: CYCLE4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-rg1zogg
