Spitzer-IRAC and NIR imaging of S255

Details Spitzer-IRAC and NIR imaging of S255 Spitzer-IRAC and NIR imaging of S255

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.6343c&link_type=abstract

American Astronomical Society Meeting 207, #63.43; Bulletin of the American Astronomical Society, Vol. 37, p.1253

Astronomy and Astrophysics

Astronomy

Scientific paper

As a part of our Spitzer GTO program we are conducting a study of eight regions of high-mass star formation with prominent photo-dissociation regions (PDR's) to investigate their content and structure. We present IRAC-Spitzer and Flamingos-NIR observations of the Massive Star Forming Region S255. We used the IRAC colors to identify young stars, to study the spatial distribution of Class I and II objects and to compare it in relation to that of the PDR. We combined IRAC + NIR data to construct the SED of stars from 1.24 to 8 μ m and to determine the persence of accretion disks in stars.

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