Deep Hα survey of the Milky Way. IV. The L = 301° to L = 324° area

Details Deep Hα survey of the Milky Way. IV. The L = 301° to L = 324° area Deep Hα survey of the Milky Way. IV. The L = 301° to L = 324° area

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..130..119r&link_type=abstract

Astronomy and Astrophysics Supplement, v.130, p.119-132

Astronomy and Astrophysics

Astrophysics

17

Interstellar Medium: Hii Regions, Galaxy: Structure

Scientific paper

The detailed velocity field of the ionized hydrogen has been observed between l = 301°\ and l = 324° as part of an Hα Survey of the southern Milky Way. Analysis of the Hα profiles shows six different velocity components. These Hα observations, combined with multiwavelength and stellar data, are used to find the most probable distances of the different gas layers. Based on observations collected at the European Southern Observatory.

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