A dataset provided by the European Space Agency

Name 7270
Title The Origin of Highly Ionized Gas in the Milky Way and Its Relationship To Large Galactic Structures
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=7270;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-pfym1mn
Author Sembach, Kenneth
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=7270&mission=hst
Publication
  • 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 Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
  • A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way
  • Atomic and Molecular Carbon as a Tracer of Translucent Clouds
  • Background and Scattered-Light Subtraction in the High-Resolution Echelle Modes of the Space Telescope Imaging Spectrograph
  • Detection in the Interstellar Medium of the Weak Mg II Transition at 1398.8 A
  • Direct Measurement of the Ratio of Carbon Monoxide to Molecular Hydrogen in the Diffuse Interstellar Medium
  • Does the Milky Way Produce a Nuclear Galactic Wind?
  • Do starburst winds escape? Insights from QSO absorption lines
  • Far Ultraviolet Spectroscopic Explorer Observations of O VI Overlying the Scutum Supershell
  • Highly-ionized gas; probing energetic galactic environments
  • Hubble Space Telescope Survey of Interstellar 12CO/13CO in the Solar Neighborhood
  • Interstellar Krypton Abundances: The Detection of Kiloparsec-scale Differences in Galactic Nucleosynthetic History
  • 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
  • STIS and GHRS Observations of Warm and Hot Gas Overlying the Scutum Supershell (GS 018-04+44)
  • The abundance of boron in diffuse interstellar clouds
  • The Abundance of Boron in Diffuse Interstellar Clouds
  • The Abundance of Interstellar Boron
  • The Interstellar N/O Abundance Ratio: Evidence for Local Infall?
  • The Variation of Magnesium Depletion with Line-of-Sight Conditions
  • Updated interstellar abundance studies and implications for dust models
Instrument STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 1998-12-23T12:43:29Z/1999-05-28T06:57:26Z
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 2006-12-20T04:38:04Z
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, Sembach comma Kenneth, 2006, 'The Origin of Highly Ionized Gas in the Milky Way and Its Relationship To Large Galactic Structures', 1.0, European Space Agency, https://doi.org/10.5270/esa-pfym1mn