A dataset provided by the European Space Agency

Name 5879
Title THE DEUTERIUM TO HYDROGEN RATIO IN THE INTERSTELLAR MEDIUM
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=5879;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-t4ep26f
Author Henry, Richard C.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=5879&mission=hst
Publication
  • Hubble Space Telescope Constraints on the Winds and Astrospheres of Red Giant Stars
  • In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
  • Lyman-Alpha Absorption and the D/H Ratio in the Local Interstellar Medium
  • Measured Mass-Loss Rates of Solar-like Stars as a Function of Age and Activity
  • The Coronae of Moderate-Mass Giants in the Hertzsprung Gap and the Clump
  • The Three-dimensional Structure of the Warm Local Interstellar Medium. II. The Colorado Model of the Local Interstellar Cloud
  • The Three-dimensional Structure of the Warm Local Interstellar Medium. I. Methodology
  • Two New Low Galactic D/H Measurements from the Far Ultraviolet Spectroscopic Explorer
  • What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument HRS, HRS/1, HRS/2
Temporal Coverage 1995-08-07T02:18:59Z/1995-09-27T06:02:37Z
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 1996-09-28T00:14:18Z
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, Henry comma Richard C., 1996, 'THE DEUTERIUM TO HYDROGEN RATIO IN THE INTERSTELLAR MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-t4ep26f