Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
A new and unusual LBV-like outburst from a Wolf-Rayet star in the outskirts of M33
HSTUV measurements of wind structure and velocities in Local Group OB stars
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
Star Clusters in M33. I. Detection, Morphology, and Photometry
Star Clusters in M33. III. The Youngest Population
Star clusters in M 33. IV. A new survey from deep HST images
The DIRECT Project: Influence of Blending on the Cepheid Distance Scale. I. Cepheids in M31
The UV-brightest Stars of M33 and Its Nucleus: Discovery, Photometry, and Optical Spectroscopy
The Winds of Hot Stars in External Galaxies. III. HST UV Spectroscopy of O and B Supergiants in M31 and M33
Instrument
FOS/BL, WFPC2, WFPC2/PC
Temporal Coverage
1994-06-29T04:23:17Z/1995-02-01T08:46:25Z
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, Bianchi et al., 1996, 'STELLAR WINDS OF MASSIVE STARS IN NEARBY GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-zfk45p3