COS-GTO: Sampling the Interstellar Gas Between the Milky Way and Triangulum Galaxies

Details COS-GTO: Sampling the Interstellar Gas Between the Milky Way and Triangulum Galaxies COS-GTO: Sampling the Interstellar Gas Between the Milky Way and Triangulum Galaxies

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11521g&link_type=abstract

HST Proposal ID #11521. Cycle 17

Physics

Scientific paper

By making interstellar absorption measurements towards the star UIT-236 located within the M33 {Triangulum} galaxy we shall be able to sample gas associated with the inner and outer halo of the Milky Way, the intergalactic medium and gas in the M33 galaxy itself. Such sight-line measurements will enable a direct determination of the velocity structure and the chemical and physical nature of both neutral and ionized gas associated with, and located between, two spiral galaxies belonging to the Local Group.;

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