A dataset provided by the European Space Agency

Name 8637
Title Distance to the prototype WD showing signatures of a super-hot wind
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8637;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-7dnts1z
Author Werner, Klaus
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8637&mission=hst
Publication
  • Metal abundances in hot white dwarfs with signatures of a superionized wind
  • Mysterious, variable, and extremely hot: White dwarfs showing ultra-high excitation lines. I. Photometric variability
Instrument STIS, STIS/CCD
Temporal Coverage 2001-01-19T06:43:35Z/2001-01-19T08:54:09Z
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 2002-01-19T08:54:09Z
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, Werner comma Klaus, 2002, 'Distance to the prototype WD showing signatures of a super-hot wind', 1.0, European Space Agency, https://doi.org/10.5270/esa-7dnts1z