Extinction Associated with the Ultracompact HII Region, S88B

Details Extinction Associated with the Ultracompact HII Region, S88B Extinction Associated with the Ultracompact HII Region, S88B

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.7103g&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #71.03; Bulletin of the American Astronomical Society, Vol. 30, p.1355

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Scientific paper

We present high spatial resolution mapping of the inner arcminute of the compact HII region S88B (G61.5+0.1) in Br gamma (2.122 micron ) line emission and compare with 5 GHz radio continuum emission (Garay et al. 1993). On a larger scale (1deg x 0.5deg ), the stellar counts derived from Two Micron All Sky Survey (2MASS) images are used to determine the extent of the molecular cloud surrounding S88B. By varying the line-of-sight extinction, we fit a spectral type to stars appearing in J (1.25 micron ), H (1.65 micron ), K (2.23 micron ) and 3.3 micron broad band images taken with the University of Rochester 3(rd) Generation Infrared Camera and compare with other extinction determinations.

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