High Resolution Observations of 6.7-GHz Methanol Masers with the LBA

Details High Resolution Observations of 6.7-GHz Methanol Masers with the LBA High Resolution Observations of 6.7-GHz Methanol Masers with the LBA

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..355d&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

We have made VLBI images of a selection of methanol masers which have
been reported to have linear structures. We find that the emission does
not lie on the expected simple velocity axis predicted by the
star-forming disk model. We suggest an alternate explanation based on a
shock in a gravitational bound star-forming core.

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