A dataset provided by the European Space Agency

Name 14081
Title Probing Supernovae Chemical Yields in Low Metallicity Environments with UV Spectroscopy of Magellanic Cloud B-type Stars
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14081;TAPCLIENT=DOI
DOI https://doi.org/10.57780/esa-mencbkx
Author Lanz, Thierry
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14081&mission=hst
Publication
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2015-12-30T12:11:09Z/2016-11-16T02:16:24Z
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 2017-11-16T05:04:21Z
Last Update 2025-01-25
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, Lanz et al., 2017, 'Probing Supernovae Chemical Yields in Low Metallicity Environments with UV Spectroscopy of Magellanic Cloud B-type Stars', 1.0, European Space Agency, https://doi.org/10.57780/esa-mencbkx