The 43 GHz SiO maser emission around the Mira variable TX Cam: 62 epoch movie of the v = 1, J = 1→0 transition.

Details The 43 GHz SiO maser emission around the Mira variable TX Cam: 62 epoch movie of the v = 1, J = 1→0 transition. The 43 GHz SiO maser emission around the Mira variable TX Cam: 62 epoch movie of the v = 1, J = 1→0 transition.

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002evn..conf..227g&link_type=abstract

6th European VLBI Network Symposium on New Developments in VLBI Science and Technology, held in Bonn, June 25th-28th 2002, proce

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have produced a new version of the movie of the v = 1, J = 1→0 43 GHz SiO maser around the Mira variable TX Cam. The new movie consists of 62 epochs, 18 more than the previous one. Observations of the masers were carried out using NRAO's Very Long Baseline Array. The VLBA is an instrument of the National Radio Astronomy Observatory, a facility of the NSF operated under cooperative agreement by Associated Universities, Inc. (VLBA) approximately every two weeks, from May 1997. The new movie covers about 1.64 stellar cycles. Gaussian fitting will give us the proper motions of the individual components and the determination of the percentage and position angle of polarisation will be used to produce the first polarisation movie.

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