Large-beam near-infrared and 24-GHz observations of M8

Details Large-beam near-infrared and 24-GHz observations of M8 Large-beam near-infrared and 24-GHz observations of M8

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..341z&link_type=abstract

Astronomical Journal, vol. 84, Mar. 1979, p. 341-344.

Astronomy and Astrophysics

Astronomy

6

Infrared Astronomy, Near Infrared Radiation, Nebulae, Radio Astronomy, Sagittarius Constellation, Astronomical Maps, Astronomical Photometry, Carbon Monoxide, Interstellar Gas, Plasma Clouds

Scientific paper

This paper presents photometric observations of M8 from 1.2 to 4.6 microns, a 3.5-micron map made with a 46-arcsec beam, and a 24.1-GHz map made with an 80-arcsec beam. A comparison with previous observations at 11 and 69 microns and of CO suggests that the radio continuum and infrared emission come from the same volume powered by the star Herschel 36. A search for the heating sources of CO Bright Spots 2 and 3 resulted in the detection of two candidates, which need additional infrared observations to ascertain their physical properties and association with the molecular cloud.

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