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Rotating Protoplanetary Gas Disk in GG-Tau
Published online by Cambridge University Press: 12 April 2016
Abstract
A rotating gas disk was discovered around a T-Tauri star, GG-Tau, in Taurus by using the Nobeyama Millimeter Array (NMA) (Kawabe et al. 1993). To analyze the observed data, we have numerically calculated velocity profiles of CO emitted from protoplanetary gas disks by taking account of the line radiative transfer.
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- 3. Astronomical Results and Prospects
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- Copyright © Astronomical Society of the Pacific 1994