Academia Sinica Institute of Astronomy & Astrophysics
中央研究院天文及天文物理研究所
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Coordinated Hydrodynamic and Astrophysical Research, Modeling, and Synthesis (CHARMS)

HIGH-RESOLUTION CO OBSERVATION OF THE CARBON STAR CIT 6
Image Credit: Hyosun Kim, Sheng-Yuan Liu, Naomi Hirano et al. (2015)
HIGH-RESOLUTION CO OBSERVATION OF THE CARBON STAR CIT 6
Radial profiles of the 12CO J = 2–1 (left panel) and 13CO J = 2–1 (right panel) emission of the carbon star CIT6 at its systemic velocity observed by the Submillimeter Array (SMA), the Submillimeter Telescope (SMT), and combined. Results from the calculations with our radiative transfer modeling package (SPARX), as overlaid by green curves, reproduced the observed profile very well.
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