Modeling the spectra of young M dwarfs

Details Modeling the spectra of young M dwarfs Modeling the spectra of young M dwarfs

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17...17l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 1, p. 17-23

Physics

1

Scientific paper

We discuss the results of modeling the optical spectra of late type stars for different molecular line lists of TiO. The synthetic spectra at lambdalambda 668.5-672.5, 768.5-772.5 and 810.5-814.5 nm were simulated using both the just overlapping line (JOLA) and "line by line" (LBL) approximations for Plez's and Shwenke's TiO line lists. From the fit of the calculated spectra to the observed ones - young PMS stars V927 Tau and FN Tau - we show that the synthetic spectra based on the Shwenke's TiO line list reproduce the observations more accurately.

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