Near Infrared Observations of the Star Formation Region AFGL 6366s

Details Near Infrared Observations of the Star Formation Region AFGL 6366s Near Infrared Observations of the Star Formation Region AFGL 6366s

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.7208m&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #72.08; Bulletin of the American Astronomical Society, Vol. 30, p.1360

Astronomy and Astrophysics

Astronomy

Scientific paper

We will provide evidence in support of the theory that the infrared cluster, AFGL 6366s, of young stellar objects contains a class B2 star, and that this object is the source of the ionization of the H II region and for the powering of the bipolar molecular outflow. This study was done in the near infrared. Broadband images of AFGL 6366s at wavelengths of J(1.25 mu m), H(1.65 mu m), K(2.23 mu m), and 3.3(3.26 mu m) as well as narrow band CVF images for Brgamma (n = 7 -> 4 , 2.166 mu m), 3.29mu m and 3.4mu m unidentified feature emission (UIR lines) are provided.

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