A dataset provided by the European Space Agency

Name 8043
Title PHYSICAL PROPERTIES OF H I AND H II REGIONS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8043;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ph1fe4g
Author Jenkins, Edward B.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8043&mission=hst
Publication
  • Abundances and Behavior of 12CO, 13CO, and C2 in Translucent Sight Lines
  • Abundances and Depletions of Interstellar Oxygen
  • Abundances and Depletions of Neutron-capture Elements in the Interstellar Medium
  • A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity
  • A New FUSE Survey of Interstellar HD
  • A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
  • Atomic and Molecular Carbon as a Tracer of Translucent Clouds
  • Cloud Structure and Physical Conditions in Star-forming Regions from Optical Observations. II. Analysis
  • Direct Measurement of the Ratio of Carbon Monoxide to Molecular Hydrogen in the Diffuse Interstellar Medium
  • Far-ultraviolet Dust Extinction and Molecular Hydrogen in the Diffuse Milky Way Interstellar Medium
  • Fundamental Properties of the Highly Ionized Plasmas in the Milky Way
  • Highly-ionized gas; probing energetic galactic environments
  • Interstellar Krypton Abundances: The Detection of Kiloparsec-scale Differences in Galactic Nucleosynthetic History
  • Is There Enhanced Depletion of Gas-Phase Nitrogen in Moderately Reddened Lines of Sight?
  • Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead
  • Measurements of the f-Values of the Resonance Transitions of Ni II at 1317.217 and 1370.132 A
  • Oxygen Gas-Phase Abundance Revisited
  • Phosphorus in the diffuse interstellar medium
  • The abundance of boron in diffuse interstellar clouds
  • The Abundance of Boron in Diffuse Interstellar Clouds
  • The Distribution of Thermal Pressures in the Interstellar Medium from a Survey of C I Fine-Structure Excitation
  • The Interstellar N/O Abundance Ratio: Evidence for Local Infall?
  • The interstellar N2 abundance towards HD 124314 from far-ultraviolet observations
  • Ultraviolet Measurements of Interstellar C2
  • Ultraviolet Survey of CO and H2 in Diffuse Molecular Clouds: The Reflection of Two Photochemistry Regimes in Abundance Relationships
  • Updated interstellar abundance studies and implications for dust models
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 1999-02-18T08:49:21Z/1999-08-07T19:45:31Z
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 2006-12-23T03:20:43Z
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, Jenkins comma Edward B., 2006, 'PHYSICAL PROPERTIES OF H I AND H II REGIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-ph1fe4g