A dataset provided by the European Space Agency

Name 8145
Title Abundances and Physical Conditions in the ISM of the Magellanic Clouds
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8145;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-4ilz7hf
Author Welty, Daniel E.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8145&mission=hst
Publication
  • Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
  • Interstellar TiII in the Milky Way and Magellanic Clouds
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • Physical conditions in the diffuse interstellar medium of local and high-redshift galaxies: measurements based on the excitation of H2 rotational and C I fine-structure levels
  • Probing the Dust Responsible for Small Magellanic Cloud Extinction
  • Thermal Pressures in the Interstellar Medium of the Magellanic Clouds
  • Unusual Depletions toward the SMC Star SK 155-Differences in Dust Composition in the SMC Interstellar Medium?
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2000-04-26T01:35:11Z/2000-10-07T23:10:14Z
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 2001-10-07T23:10:14Z
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, Welty comma Daniel E., 2001, 'Abundances and Physical Conditions in the ISM of the Magellanic Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-4ilz7hf