The Emitted Spectrum of a Proto-Star
Open Access
- 1 August 1969
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 145 (3) , 297-308
- https://doi.org/10.1093/mnras/145.3.297
Abstract
The spectral energy distribution emitted by a collapsing proto-star has been calculated on the basis of some simple approximations for the radiative transfer in the extended spherical ‘ atmosphere ’ of the proto-star. Results for the evolution in spectral appearance are presented for several of the collapsing proto-star calculations described in a previous paper (Larson 1969). Comparison is made with some observations of infra-red objects in Orion and with recent infra-red observations of T Tauri stars.Keywords
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