A Measurement of Proper Motions of SiO Maser Sources in the Galactic Center with the VLBA

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

High-res. figures are available at ftp://ftp.nro.nao.ac.jp/nroreport/no656.pdf.gz . PASJ 60, No. 1 (2008) in press

Scientific paper

We report on the high-precision astrometric observations of maser sources around the Galactic Center in the SiO J=1--0 v=1 and 2 lines with the VLBA during 2001 -- 2004. With phase-referencing interferometry referred to the radio continuum source Sgr A*, accurate positions of masers were obtained for three detected objects: IRS 10 EE (7 epochs), IRS 15NE (2 epochs), and SiO 6 (only 1 epoch). Because circumstellar masers of these objects were resolved into several components, proper motions for the maser sources were derived with several different methods. Combining our VLBA results with those of the previous VLA observations, we obtained the IRS 10EE proper motion of 76+-3 km s^{-1} (at 8 kpc) to the south relative to Sgr A*. Almost null proper motion of this star in the east--west direction results in a net transverse motion of the infrared reference frame of about 30+-9 km s^{-1} to the west relative to Sgr A*. The proper-motion data also suggests that IRS 10EE is an astrometric binary with an unseen massive companion.

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

A Measurement of Proper Motions of SiO Maser Sources in the Galactic Center with the VLBA 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 A Measurement of Proper Motions of SiO Maser Sources in the Galactic Center with the VLBA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Measurement of Proper Motions of SiO Maser Sources in the Galactic Center with the VLBA will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-300606

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