Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, WFPC2, WFPC2/PC
Temporal Coverage
2000-09-29T20:17:19Z/2001-01-07T04:35:36Z
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, Bruhweiler, 2006, 'The Search for True'' Starburst Dust and the Importance of Metallicity on Properties of O & B Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-hh8nlz3