Micro-arcsec Astrometry of the Milky Way and Beyond

Details Micro-arcsec Astrometry of the Milky Way and Beyond Micro-arcsec Astrometry of the Milky Way and Beyond

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..34...53r&link_type=abstract

IV Reunión sobre Astronomía Dinámica en Latino América (Eds. C. Allen, A. Ruelas, & R. Teixeira) Revista Mexicana de Astronomía

Astronomy and Astrophysics

Astronomy

Astrometry, Galaxy: Structure, Stars: Formation

Scientific paper

Recently we have been able to achieve parallaxes and proper motions with accuracies approaching micro-arcseconds using the VLBA. The apparent proper motion of Sgr A* has been measured with extremely high accuracy, strongly constraining Θ_{0}/R_0 and potentially offering a new dynamical definition of the Galactic plane. The intrinsic motion of Sgr A* perpendicular to the Galactic plane is extremely small (˜ 1 km s^{-1}) and comparable to that expected for a supermassive black hole. When coupled with IR observations of stellar orbits, this provides overwhelming evidence for the existence of supermassive black holes. We have measured trigonometric parallaxes and proper motions for about a dozen high-mass star forming regions (HMSFRs). Generally, kinematic distances exceed the true distances, suggesting that the IAU Galactic parameters, R_0 and Θ_{0}, may need modification. Values of the Solar Motion from our data agree with those obtained from Hipparcos data, but HMSFRs appear to be rotating slower than the Galaxy. Finally, the extraordinary astrometric capabilities of the VLBA have been used to measure extragalactic proper motions and to map masers in distant AGN accretion disks, which will yield direct estimates of H_0.

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