Abstracts, Galactic Center Workshop '98
GCNEWS
A Newsletter for Galactic Center Research
This Volume was edited by Angela Cotera & Heino Falcke
email: gcnews@aoc.nrao.edu

ABSTRACT

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Proper Motions and Structure of the Radio Components near Sgr A*
Jun-Hui Zhao 1 , W. M. Goss 2
1 Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS 78, Cambridge, MA 02138; 2 NRAO-AOC, P. O. Box O, Socorro, NM 87801;
ABSTRACT:
Proper motions and radio structure of the HII component near Sgr A*
have been determined based on high resolution (0.1") observations at
13 and 7 mm in the past 7 years (1991-1998). Large proper motions up
to 30 mas/yr (or 1200 km/s) have been observed for a number of
prominent features. The large proper motion measured from the compact
HII components can be explained by motions of a clumpy HII gas
accelerated by either strong winds and outflows or explosive events at
the Galactic center. Large pattern speeds due to wave or shock
motions in the circumnuclear medium at the Galactic center can also be
responsible for part of the observed proper motions. In addition, the
HII components near Sgr A* (within the central 2.5" or 0.1 pc) show
filamentary structures suggesting that the HII components are tidally
disrupted by tides due to the concentration of mass at the Galactic
center. High precision measurements of the proper motions for these
HII components can be used to track the motions of the accreting gas
in close proximity to the super massive black hole apparently
associated with Sgr A*.
LINKS: Program, Author, jzhao@cfa.harvard.edu
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File last modified on Monday 04 August 2003 [10:43 MDT].
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