H166α Emission as a Tracer of the Warped Ionized Gas Layer in the Northern Galaxy

Details H166α Emission as a Tracer of the Warped Ionized Gas Layer in the Northern Galaxy H166α Emission as a Tracer of the Warped Ionized Gas Layer in the Northern Galaxy

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.253..313a&link_type=abstract

Astrophysics and Space Science, Volume 253, Issue 2, pp.313-323

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

Observations of the H166 α recombination line were made with the 43 m antenna of the National Radio Astronomy Observatory (NRAO), in Green Bank, West Virginia, United States of America. The United States of results of the observations in the galactic longitude range 60-

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