Astrometry of W49N - OH43.8-0.1 H2O maser pair with VERA

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2 pages. 1 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Edito

Scientific paper

We present the results of multi-epoch VERA observations of W49N - OH43.8-0.1 water maser pair. Based on the dual-beam VLBI observation with VERA, we successfully obtained the phase-referenced maps of OH43.8-0.1 with respect to the W49N reference spot for 3 epochs with a time span of 6 months. The maps were in good agreement with previous studies obtained with a single-beam VLBI, and were also consistent with each other with an accuracy of about 0.2 mas. Moreover, there are systematic, rather linear displacements of maser feature positions, which may be the relative proper motions of maser features caused by the Galactic rotation as well as internal motions of individual maser features.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Astrometry of W49N - OH43.8-0.1 H2O maser pair with VERA does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Astrometry of W49N - OH43.8-0.1 H2O maser pair with VERA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrometry of W49N - OH43.8-0.1 H2O maser pair with VERA will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-45225

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.