Characterizing the Stellar Population in NGC 1705-1
Characterizing Transition Temperature Gas in the Galactic Corona
From young massive star cluster to old globular: the LV-s0 relationship as a diagnostic tool
Massive Star Formation in the Ultraviolet Observed with the Hubble Space Telescope
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Super Star Cluster NGC 1705-1: A Local Analog to the Birth Site of Long-Duration g-Ray Bursts
The Lya Forest of a Lyman Break Galaxy: Very Large Telescope Spectra of MS 1512-cB58 at z=2.724
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-06-11T03:02:51Z/2000-07-31T11:51:40Z
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, Leitherer comma Claus, 2001, 'The Physical State of the Starburst Outflow in NGC1705', 1.0, European Space Agency, https://doi.org/10.5270/esa-5i0yap6