Exploring milliarcsec-scale structures using spectro-astrometry

Details Exploring milliarcsec-scale structures using spectro-astrometry Exploring milliarcsec-scale structures using spectro-astrometry

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..799t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 12, p. 799 - 807 (2005)

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Milliarcsec-Scale Structures, Spectro-Astrometry

Scientific paper

Observations with high-angular resolutions have always provided exciting results to understand stars, galaxies, proto-planetary disks etc. Interferometers such as VLTI and Keck have begun to explore milli-arcsec structures at optical-IR wavelengths in additions to radio wavelengths. We have used another approach - namely "Spectro-astrometry" - to explore milliarcsec-scale structures. In this article I review its concept, our results to date and a possibility to explore micro-arcsec scales in the future.

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