A dataset provided by the European Space Agency

Name 8273
Title The Oxygen Abundance in Translucent Interstellar Clouds
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8273;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-uuaj1w5
Author Meyer, David M.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8273&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
  • Broadened profiles of diffuse interstellar bands
  • Cloud Structure and Physical Conditions in Star-forming Regions from Optical Observations. II. Analysis
  • Determining Interstellar Carbon Abundances from Strong-line Transitions
  • Direct Measurement of the Ratio of Carbon Monoxide to Molecular Hydrogen in the Diffuse Interstellar Medium
  • High-resolution ultraviolet spectroscopy of gas in galaxy halos and large-scale structures
  • Hubble Space Telescope Survey of Interstellar 12CO/13CO in the Solar Neighborhood
  • Interstellar H2 toward HD 147888
  • Interstellar H2 toward HD 37903
  • Interstellar Medium in the M43 Nebula
  • Is There Enhanced Depletion of Gas-Phase Nitrogen in Moderately Reddened Lines of Sight?
  • Physical Conditions in Orions Veil. II. A Multicomponent Study of the Line of Sight toward the Trapezium
  • Potential Variations in the Interstellar N I Abundance
  • Probing the Role of Carbon in Ultraviolet Extinction along Galactic Sight Lines
  • Space Telescope Imaging Spectrograph Observations of Interstellar Oxygen and Krypton in Translucent Clouds
  • The Distribution of Metallicities in the Local Galactic Interstellar Medium
  • The Homogeneity of Interstellar Elemental Abundances in the Galactic Disk
  • The Rich Ultraviolet Spectrum of Vibrationally Excited Interstellar H2 toward HD 37903
  • The Transition from Diffuse Molecular Gas to Molecular Cloud Material in Taurus
  • 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
  • Vibrationally Excited Molecular Hydrogen near Herschel 36
Instrument STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2000-01-23T00:43:53Z/2000-10-30T17:21:37Z
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 2006-12-20T13:09:58Z
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, Meyer comma David M., 2006, 'The Oxygen Abundance in Translucent Interstellar Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-uuaj1w5