Chemical Abundances and Properties of the Ionized Gas in NGC 1705
Chemical abundances of two extragalactic young massive clusters
Compact Star Clusters in Nearby Dwarf Irregular Galaxies
Far-Ultraviolet Observations of Molecular Hydrogen in the Diffuse Interstellar Medium of Starburst Galaxies
Homogenization of the Stellar Population along Late-Type Spiral Galaxies
Structural Properties of Massive Young Clusters
The Resolved Stellar Populations in NGC 1705
The Star Formation History of NGC 1705: A Poststarburst Galaxy on the Verge of Activity
Young Stellar Populations and Star Clusters in NGC 1705
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-03-04T21:56:13Z/2000-11-11T13:55:33Z
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, Tosi et al., 2001, 'NGC 1705: a Benchmark for Galaxy Evolution', 1.0, European Space Agency, https://doi.org/10.5270/esa-imtq49s