The VLBA Survey of OH Masers towards SFR: Preliminary Results

Details The VLBA Survey of OH Masers towards SFR: Preliminary Results The VLBA Survey of OH Masers towards SFR: Preliminary Results

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..361m&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

Scientific paper

In 2001 the VLBA was used as part of a continuing program to observe OH MASERs towards Star Forming Regions, to study their structure with the highest angular resolution possible. One goal is to classify the sources by their structure and prepare a database composed of those that show highly compact structure and promise interesting and exciting results when observed with higher resolution arrays (i.e. Space-VLBI). We present preliminary results from the first 45 sources observed. These are the first high resolution observations for over 50% of the sources. Approximately 20% exhibit highly compact structure and moderately strong emission.

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