Abstract
We present a study of weak near-IR absorption lines in 44 low luminosity YSOs. Using a spectral resolution of ~ 1000 most Class II sources show CO overtone absorption bands of varying strength in the K window, whether they have optical counterparts or not. Class I sources tend to show featureless 2 μm continua even though a S/N > 100 was achieved. High resolution (R=17000) echelle spectra were also obtained for a sub-sample of YSOs. Most show an unresolved 12CO(2–0) bandhead, which when combined with inferred CO excitation temperatures and optical depths clearly points to a photospheric rather than a disk origin for the bands. They also show that embedded Class Its are not rapidly rotating.
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References
Casali, M. & Matthews, H.: 1992, Mon. Not. of the RAS 258, 399.
Hodapp, K. & Deane, J.: 1993, Astrophys. J., Suppl. 88, 119.
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© 1995 Springer Science+Business Media Dordrecht
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Casali, M.M., Eiroa, C. (1995). Near-IR Spectroscopy and the Photospheres of Embedded YSOs. In: Watt, G.D., Williams, P.M. (eds) Circumstellar Matter 1994. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0147-9_3
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DOI: https://doi.org/10.1007/978-94-011-0147-9_3
Publisher Name: Springer, Dordrecht
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