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Spectral Line Formation in YY Ori and T Tau Envelopes
Published online by Cambridge University Press: 12 April 2016
Extract
First results of line profile computations in a collapsing rotating envelope are discussed. As an application, an observed profile of the YY Ori star CoD -35° 10525 is compared to computed profiles. Possible similarities in the formation of YY Ori and T Tau line profiles are briefly mentioned.
- Type
- Part I: Young Objects
- Information
- Copyright
- Copyright © Veröff. Der Remeis-Sterwarte 1977