A dataset provided by the European Space Agency

Name 14712
Title HST-COS Ultraviolet Spectroscopy of Be Supergiant Stars in the Magellanic Clouds
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14712;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sbj4pjr
Author Sahai, Raghvendra
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14712&mission=hst
Publication
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
Instrument COS, COS/FUV, COS/NUV, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2017-08-25T22:13:05Z/2018-01-21T21:35:55Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2019-01-21T23:10:01Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Sahai comma Raghvendra, 2019, 'HST-COS Ultraviolet Spectroscopy of B[e] Supergiant Stars in the Magellanic Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-sbj4pjr