H, H2, CO, H2O In A Sample Of Fu Ori Stars

Details H, H2, CO, H2O In A Sample Of Fu Ori Stars H, H2, CO, H2O In A Sample Of Fu Ori Stars

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aas...212.0804l&link_type=abstract

American Astronomical Society, AAS Meeting #212, #8.04; Bulletin of the American Astronomical Society, Vol. 40, p.199

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We present spectral data from a small sample of FU Ori stars. High-resolution spectra spanning 2-5 microns were taken with the NIRSPEC spectrograph on the Keck II telescope. These data were examined for near-IR spectral features, targeting H2, H, CO and H2O lines which are characteristic of this class of objects. Even within such a small sample, different spectral properties among the observed objects point to a need for further class modeling to explain absorption/emission features around 5 microns. The K, M and L band data will be presented. We find no correlation between the flux of Br-gamma and other circumstellar diagnostics.

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