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    • Keywords


      ISM: clouds, structure; radio lines: ISM

    • Abstract


      This investigation is aimed at clarifying the nature of the interstellar gas seen in absorption against bright O and B stars. Towards this end we have obtained for the first time HI absorption spectra towards radio sources very close to the lines of sight towards twenty five bright stars previously studied. In this paper we describe the selection criteria, the details regarding our observations, and finally present the absorption spectra. In the accompanying paper we analyse the results and draw conclusions.

    • Author Affiliations


      Jayadev Rajagopal1 G. Srinivasan1 K. S. Dwarakanath1

      1. Raman Research Institute, Bangalore - 560 080, India
    • Dates

  • Journal of Astrophysics and Astronomy | News

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      Posted on January 27, 2016

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