Titlebook: Circumstellar Matter 1994; Proceedings of an In G. D. Watt,P. M. Williams Conference proceedings 1995 Springer Science+Business Media Dordr

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lymphedema

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Fracture

https://doi.org/10.1007/978-3-322-99358-8environments of low to intermediate mass stars. Depletions of gas-phase molecules, grain mantle evaporation, and shock interactions actively drive chemical processes in different regions around young stars. We present results for two systems, IRAS 05338-0624 and NGC 1333 IRAS 4, to illustrate the be

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https://doi.org/10.1007/978-3-322-99358-8compared with line intensities of C.O and H.CO. We include in this analysis results from other sub-mm continuum surveys of compact HII regions, T-Tauri stars and class 0 YSO’s. The results provide a statistical sample of the long-wavelength dust spectra of ∼ 60 Young Stellar Objects. Data are displa

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https://doi.org/10.1007/978-3-8350-9166-5tellar disks around young stars. The CO emission flux and the detailed shape of the overtone bands are well matched by simple Keplerian disk models. A brief overview of the use of infrared CO emission as a diagnostic of the kinematics and conditions of gas in the inner disks of young stars is presented.