Observations and Modeling of Lynds Dark Nebula 1221

Details Observations and Modeling of Lynds Dark Nebula 1221 Observations and Modeling of Lynds Dark Nebula 1221

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.6216y&link_type=abstract

American Astronomical Society, AAS Meeting #211, #62.16; Bulletin of the American Astronomical Society, Vol. 39, p.850

Astronomy and Astrophysics

Astronomy

Scientific paper

We present observations and modeling of the Lynds Dark Nebula 1221. The observations include MIPS and IRAC data from the Spitzer Space Telescope, submillimeter continuum from the JCMT, and 2MASS near-infrared data. In addition, IRS low-resolution spectra and FCRAO molecular line observations are shown. Modeling of the continuum radiation gives a best-fit model to the data that describes the nature of the three protostars present in this low-mass star-forming region.
C. Young thanks the Louisiana Board of Regents, BoRSF, under agreement NASA/LEQSF(2001-2005)-LaSPACE and NASA/LaSPACE under grant NGT5-40115 for support during this project

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