Hostname: page-component-7479d7b7d-k7p5g Total loading time: 0 Render date: 2024-07-12T08:36:08.735Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  26 May 2016

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

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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