A dataset provided by the European Space Agency

Name 15837
Title The HST follows galactic influencers: a COS UV survey of the most massive O-stars in the SMC
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15837;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-jvjjdo6
Author Oskinova, Lidia
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15837&mission=hst
Publication
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
Instrument COS, COS/FUV, COS/NUV, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2020-04-27T10:21:13Z/2020-10-02T08:02:57Z
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 2020-10-02T17:31:20Z
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, Oskinova comma Lidia, 2020, 'The HST follows galactic influencers: a COS UV survey of the most massive O-stars in the SMC', 1.0, European Space Agency, https://doi.org/10.5270/esa-jvjjdo6