Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
Extensive observational evidence for massive star stellar wind variability at low metallicities: implications for mass-loss rate determination
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-03-12T03:06:03Z/2015-07-13T16:26:07Z
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, Roman-Duval, 2015, 'Third COS FUV Lifetime Position: Wavelength and Resolution Calibration (LCAL2)', 1.0, European Space Agency, https://doi.org/10.5270/esa-rgat6by
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.