Near-infrared observations of S 106-IRS 9

Details Near-infrared observations of S 106-IRS 9 Near-infrared observations of S 106-IRS 9

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...141..263e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 141, no. 1, Dec. 1984, p. 263-265.

Astronomy and Astrophysics

Astrophysics

1

Infrared Spectra, Infrared Stars, Interstellar Extinction, M Stars, Molecular Clouds, Stellar Spectrophotometry, Absorption Spectra, Giant Stars, Near Infrared Radiation, Nebulae, Spectral Energy Distribution

Scientific paper

1 - 5 μm photometry and 2 - 4 μm spectral photometry of the infrared source S 106-IRS 9 are reported. The observed energy distribution together with the absorption bands of CO and H2O in the infrared spectrum show that IRS 9 is a very reddened late type M giant star, which suffers high extinction produced by the S 106 molecular cloud. The distance to IRS 9 is greater than 1 kpc and thus, it is physically unrelated to the star formation region S 106.

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