SiO outflow signatures toward massive young stellar objects with linearly distributed methanol masers-Reference-Cited by-同舟云学术

SiO outflow signatures toward massive young stellar objects with linearly distributed methanol masers

Published:2008-11-06 Issue:1 Volume:493 Page:127-143
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

De Buizer J. M.,Redman R. O.,Longmore S. N.,Caswell J.,Feldman P. A.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:200810907/pdf

Reference51 articles.

1. Arce, H. G., Shepherd, D., Gueth, F., et al. 2007, in Protostars and Planets V, ed. B. Reipurth, D. Jewitt, & K. Keil (Tucson; University of Arizona Press), 245

2. Enhanced Chemical Abundances in the L1157 Outflow: SiO and CH 3OH Observations

3. Ring shaped 6.7 GHz methanol maser emission around a young high-mass star

4. CH3OH and H2O masers in high-mass star-forming regions

5. Accretion Signatures from Massive Young Stellar Objects

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