Using ISO Spectra to Interpret Colours and SEDs of YSOs Observed by Spitzer.

Details Using ISO Spectra to Interpret Colours and SEDs of YSOs Observed by Spitzer. Using ISO Spectra to Interpret Colours and SEDs of YSOs Observed by Spitzer.

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20510906k&link_type=abstract

American Astronomical Society Meeting 205, #109.06; Bulletin of the American Astronomical Society, Vol. 36, p.1533

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have used the ISO archives to assemble a sample of LWS and SWS spectra for YSOs over a range of types and evolutionary statuses. We have then derived Spitzer IRAC and MIPS band fluxes from this sample of objects of known type, and constructed Spitzer equivalent colour-colour plots and SEDs. These are used to interpret the wealth of information that is being produced by the Spitzer Space Telescope in observations of star forming regions. We compare the results to published Spitzer observations of YSOs, and to data from the Spitzer Galactic First Look Survey.

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