YSOs in L1630N and L1641 (Fang+, 2009)

Details YSOs in L1630N and L1641 (Fang+, 2009) YSOs in L1630N and L1641 (Fang+, 2009)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35040461f&link_type=abstract

VizieR On-line Data Catalog: J/A+A/504/461. Originally published in: 2009A&A...504..461F

Computer Science

Molecular Clouds, Stars: Pre-Main Sequence, Ysos, Photometry: Infrared, Equivalent Widths

Scientific paper

We performed a large optical spectroscopic and photometric survey of the aforementioned clouds. Spectral types, as well as accretion and outflow characteristics, are derived from our VLT/VIMOS spectra. Optical SDSS and CAHA/LAICA imaging was combined with 2MASS, Spitzer IRAC, and MIPS imaging to obtain spectral energy distributions from 0.4 to 24um. Reddened model atmospheres were fitted to the optical/NIR photometric data, keeping Teff fixed at the spectroscopic value. Mass and age estimates of individual objects were made through placement in the HR diagram and comparison to several sets of pre-main sequence evolutionary tracks.
************************************************************************** * * * Sorry, but the author(s) never supplied the tabular material * * (tables 8-9, 12-15) as announced in the paper * * * **************************************************************************
(7 data files).

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