A dataset provided by the European Space Agency

Name 8595
Title Does the D/H Ratio Vary in Local Interstellar Gas?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8595;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-npiq9xb
Author Sahu, Meena
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8595&mission=hst
Publication
  • Heavy-element abundance patterns in hot DA white dwarfs
  • O/H in the Local Bubble
  • The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
  • The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
  • What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2001-03-14T14:10:52Z/2001-05-03T18:37:16Z
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 2006-12-11T07:35:56Z
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, Sahu et al., 2006, 'Does the D/H Ratio Vary in Local Interstellar Gas?', 1.0, European Space Agency, https://doi.org/10.5270/esa-npiq9xb