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Formation of protoplanetary with radiation of SiO maser from Orion-IRC2

Published online by Cambridge University Press:  26 May 2016

Zhi-Yao Yu
Zhi-Yao Yu*
Affiliation:
Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, China National Astronomical Observatories, CAS, China

Abstract

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Here we report a study of formation of protoplanetary with radiation of SiO maser from Orion-IRC2 using a new model, i.e. the distinct multiple rotating and expanding disc-rings of Orion-IRC2 SiO (ν =1, J-2-1) maser for explanation of the fact that the several small peaks superposed the double-peaked spectral profile and the relative position map.

Type
Part IV: Protoplanetary and β Pic disks
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 402 - 405
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Barvainis, R. 1984, ApJ, 279, 358.Google Scholar
Plambeck, R.L., Wright, M.C.H., & Carlatrom, J.E. 1990, ApJ, 348, L65.Google Scholar
Yu, Z. 1994, Acta Astrophysica Sinica, 14, 66.Google Scholar