Identification of the 100-micron sources in CYG X

Details Identification of the 100-micron sources in CYG X Identification of the 100-micron sources in CYG X

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177p.113e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Dec. 1976, p. 113P-116P.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Maps, Far Infrared Radiation, Infrared Astronomy, Radio Sources (Astronomy), Submillimeter Waves, Astronomical Spectroscopy, Astrophysics, Balloon-Borne Instruments, H Ii Regions, Spectroscopic Telescopes

Scientific paper

The 100-micron objects HFE 64-70 detected by Hoffmann, Frederick, and Emery (1971) in Cyg X are identified with the H II regions DR 5, 6, 7, 17, 21, 22, and 23, respectively. These H II regions have higher emission measures than those not detected at 100 microns (excepting DR 13 and 25 which should be promising candidates for far-infrared emission) and are presumably younger.

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