A peculiar object in M 51: fuzzy star cluster or a background galaxy?
Gravitational torques imply molecular gas inflow towards the nucleus of M 51
High-Mass, OB Star Formation in M51: Hubble Space Telescope Ha and Paa Imaging
Identification of the Red Supergiant Progenitor of Supernova 2005cs: Do the Progenitors of Type II-P Supernovae Have Low Mass?
Molecular Gas Evolution Across a Spiral Arm in M51
Multi-transition Study of M51S Molecular Gas Spiral Arms
Star Formation and Asymmetry in the Spiral Arms of M51: Variable Star Formation Caused by More than One Spiral Density Wave
Star Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law
Star Formation in NGC 5194 (M51a): The Panchromatic View from GALEX to Spitzer
The Calibration of Mid-Infrared Star Formation Rate Indicators
The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters
The Spatially Resolved Star Formation Law From Integral Field Spectroscopy: VIRUS-P Observations of NGC 5194
The star cluster population of M 51. II. Age distribution and relations among the derived parameters
The star cluster population of M 51. III. Cluster disruption and formation history
Instrument
NICMOS, NICMOS/NIC2, NICMOS/NIC3
Temporal Coverage
1997-09-08T15:06:29Z/1997-09-08T15:10:29Z
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.
