Constraining Pre-Main-Sequence Evolutionary Tracks via Near/Mid-Infrared Observations of Young Binaries

Details Constraining Pre-Main-Sequence Evolutionary Tracks via Near/Mid-Infrared Observations of Young Binaries Constraining Pre-Main-Sequence Evolutionary Tracks via Near/Mid-Infrared Observations of Young Binaries

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.1806b&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #18.06; Bulletin of the American Astronomical Society, Vol. 32, p.1434

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results of a mid-infrared imaging photometric survey of the young, embedded population of the nearby (d=125 pc) Rho Oph molecular cloud core for binaries/multiple systems in the 0.3-10 arcsec separation range. One triple system, WL20, will be used as an illustrative example of how the combination of spatially resolved multiwavelength photometry (spanning 1--25 microns) with spatially resolved near-infrared spectroscopy of the individual components, can be used to test and constrain current pre-main-sequence evolutionary models.

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