Proposal code

v114

Proposal title

VSOP mapping of maser spots

The

Investigators and their

Affiliations

P.I. Yasuhiro Murata ISAS, Japan
Katsunori Shibata NAO, Japan
Hideyuki Kobayashi ISAS, Japan
Tomofumi Umemoto NAO, Japan
Shinji Horiuchi NAO, Japan
Kenta Fujisawa ISAS, Japan
Kiyoaki Wajima ISAS, Japan
Takahiro Iwata Communication Research Lab., Kashima, Japan
Rey Furuya Ibaragi University, Japan

Proposal Abstract

We will observe well-known star forming regions to investigate the intrinsic structure of the maser spots. We selected 6 strong water maser sources closer than 1 kpc, to avoid the interstellar scatterring. Purpose of this observation is to get high resoluton / high dynamic range maps for the water maser spots. Output of this observation will be used not only for studying each source, but used as the basic data for study of maser emission mechanisum and the study of the astronomical objects which has the maser emission.

The full Cover Sheets (compressed post-script, typically 50kbytes) can be retrieved. Note that many proposals were reduced in extent by the Scientific Review Committee (e.g. by reducing the number of experiments), however the Cover Sheets contain the full proposal as submitted. Also note that AO1 proposals were submitted in November 1995, and information such as affiliations and contact details has changed for some proposers since that time. The Cover Sheets (and the details on this page, which were derived from the Cover Sheets) may therefore have changed.