Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-25T16:06:29.135Z Has data issue: false hasContentIssue false

The VLBI mapping survey of the 6.7 GHz methanol masers with the JVN/EAVN

Published online by Cambridge University Press:  24 July 2012

K. Fujisawa
Affiliation:
The Research Institute of Time Studies, Yamaguchi Univ., 1677-1 Yoshida, Yamaguchi, Yamaguchi 753-8511, Japan email: [email protected]
K. Hachisuka
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
K. Sugiyama
Affiliation:
Dept. of Physics, Yamaguchi Univ., 1677-1 Yoshida, Yamaguchi, Yamaguchi 753-8512, Japan
A. Doi
Affiliation:
Institute of Space and Astronautical Science, JAXA, Yoshinodai 3-1-1, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
M. Honma
Affiliation:
Mizusawa VLBI Observatory, NAOJ, Hoshigaoka-cho 2-12, Oshu, Iwate 023-0861, Japan
Y. Yonekura
Affiliation:
Center for Astronomy, Ibaraki Univ., 2-1-1 Bunkyo, Mito, Ibaraki 310-8512, Japan
T. Hirota
Affiliation:
Mizusawa VLBI Observatory, NAOJ, Hoshigaoka-cho 2-12, Oshu, Iwate 023-0861, Japan
S. Sawada-Satoh
Affiliation:
Mizusawa VLBI Observatory, NAOJ, Hoshigaoka-cho 2-12, Oshu, Iwate 023-0861, Japan
Y. Murata
Affiliation:
Institute of Space and Astronautical Science, JAXA, Yoshinodai 3-1-1, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
K. Motogi
Affiliation:
Dept. of Cosmosciences, Hokkaido Univ., N10 W8, Sapporo 060-0810, Japan
H. Ogawa
Affiliation:
Graduate School of Science, Osaka Pref. Univ., 1-1 Gakuen-cho, Nakaku, Sakai, Osaka 599-8531, Japan
X. Chen
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
K.-T. Kim
Affiliation:
Korea Astronomy and Space Science Institute, Hwaam-Dong, Yuseong-Gu, Daejeon 305-348, Korea
Z.-Q. Shen
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
Rights & Permissions [Opens in a new window]

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.

We present VLBI maps of the 6.7 GHz methanol maser emission in 32 sources obtained using the Japanese VLBI Network (JVN) and the East-Asian VLBI Network (EAVN). All of the observed sources provide new VLBI maps, and the spatial morphologies have been classified into five categories similar to the results obtained from European VLBI Network observations (Bartkiewicz et al. 2009). The 32 methanol sources are being monitored to measure the relative proper motions of the methanol maser spots.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Bartkiewicz, A., Szymczak, M., van Langevelde, , et al. 2009 A&A, 502, 155Google Scholar
Caswell, J. L., Fuller, G. A., Green, J. A., et al. 2010, MNRAS, 404, 1029Google Scholar
Goddi, C., Moscadelli, L., & Sanna, A. 2011, A&A, 535, L8Google Scholar
Green, J. A., Caswell, J. L., Fuller, G. A., et al. 2010, MNRAS, 409, 913Google Scholar
Moscadelli, L., Cesaroni, R., Rioja, M. J., et al. 2011, A&A, 526, A66Google Scholar
Pestalozzi, M. R., Minier, V., & Booth, R. S. 2005, A&A, 432, 737Google Scholar
Robitaille, T. P., Whitney, B. A., Indebetouw, R., et al. 2006, ApJS, 167, 256Google Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010a, A&A, 517, A71Google Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010b, A&A, 517, A78Google Scholar