Red MSX Survey (RMS): bolometric fluxes of YSOs (Mottram+, 2011)

Details Red MSX Survey (RMS): bolometric fluxes of YSOs (Mottram+, 2011) Red MSX Survey (RMS): bolometric fluxes of YSOs (Mottram+, 2011)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35259149m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/525/A149. Originally published in: 2011A&A...525A.149M

Physics

Surveys, H Ii Regions, Ysos, Stars: Pre-Main Sequence, Millimetric/Submm Sources

Scientific paper

We use a model spectral energy distribution (SED) fitter to obtain the bolometric flux for our sources, given flux data from our work and the literature. The inputs to the model fitter were optimised by a series of investigations designed to reveal the effect varying these inputs had on the resulting bolometric flux. Kinematic distances derived from molecular line observations were then used to calculate the luminosity of each source.
(2 data files).

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