A dataset provided by the European Space Agency

Name 13781
Title WO-Type Wolf-Rayet Stars: the Last Hurrah of the Most Massive Stars?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13781;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sst7f3n
Author Massey, Philip Louis
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13781&mission=hst
Publication
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • WO-type Wolf-Rayet Stars: The Last Hurrah of Massive Star Evolution
Instrument COS, COS/FUV, COS/NUV, STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2015-07-04T16:13:40Z/2015-07-16T14:44:56Z
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 2016-07-17T16:16:49Z
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, Massey comma Philip Louis, 2016, 'WO-Type Wolf-Rayet Stars: the Last Hurrah of the Most Massive Stars?', 1.0, European Space Agency, https://doi.org/10.5270/esa-sst7f3n