A near-infrared study of the region L = 305 deg

Details A near-infrared study of the region L = 305 deg A near-infrared study of the region L = 305 deg

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132..301d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. 301-311.

Astronomy and Astrophysics

Astronomy

14

Galactic Structure, Infrared Astronomy, Spiral Galaxies, Astronomical Photometry, Galactic Clusters, Interstellar Masers, Molecular Clouds, Nebulae

Scientific paper

The structure of the Sagittarius spiral arm is studied through the combination of radio observations, near-IR photography, spectroscopy, and IR photometry in the direction of l = 305 deg, b = 0.2. An unambiguous identification of 11 sources as M stars ranging in distance from 1 to 3.8 kpc has been accomplished, and many of the 72 sources studied have been found to be members of two new galactic clusters. Three sources are identified as the IR components of OH/H2O masers.

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