The Scutum ring of H II regions

Details The Scutum ring of H II regions The Scutum ring of H II regions

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..127h&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astronomy

H Ii Regions, Radio Sources (Astronomy), Scutum Constellation, Stellar Evolution, Carbon Monoxide, Continuous Spectra, H Lines, Ionized Gases

Scientific paper

Radio continuum, H I line, and CO line observations presented suggest that the ring of compact radio continuum sources found at l = 24.6 deg, b = 0.0 deg, and presently designated the 'Scutum ring', is a star-forming region triggered by an expanding, diffuse H II region. This triggering mechanism has been suggested as a model for sequential star formation by Elmegreen and Lada (1977); the Scutum ring may be in a later phase of a Rosette nebula-type structure.

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