A dataset provided by the European Space Agency

Name 1190
Title FUV EMISSION LINE PROFILES OF W SERPENTIS BINARIES: CYCLE 1 OBSERVATIONS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=1190;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-fz55f1r
Author Beaver, Edward A.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=1190&mission=hst
Publication
  • Goddard High-Resolution Spectrograph Observations of the Interacting Binary System W Serpentis
  • Non-conservative evolution in Algols: where is the matter?
Instrument HRS, HRS/2
Temporal Coverage 1991-07-12T02:43:23Z/1991-07-19T04:05:52Z
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 1992-07-18T21:13:25Z
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, Beaver comma Edward A., 1992, 'FUV EMISSION LINE PROFILES OF W SERPENTIS BINARIES: CYCLE 1 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-fz55f1r