An updated survey of globular clusters in M 31. II. Newly discovered bright and remote clusters
Detection of a 100,000 M black hole in M31s Most Massive Globular Cluster: A Tidally Stripped Nucleus
Evidence for metallicity spreads in three massive M 31 globular clusters
Modelling of integrated-light spectra from the optical to the near-infrared: the globular cluster G280 in M31
On the Progenitors of Local Group Novae. II. The Red Giant Nova Rate of M31
On the Progenitors of Local Group Novae. I. The M31 Catalog
Structural Parameters for Globular Clusters in M31 and Generalizations for the Fundamental Plane
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-08-06T11:22:08Z/2003-09-14T10:01:01Z
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, Bridges comma Terry, 2004, 'Metallicity Spreads in M31 Globular Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-rb1iem4