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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Radio Recombination Lines near lambda = 20 cm from the Sgr A Complex
Anantharamaiah, K.R.1,3; Pedlar, A.2; Goss, W.M.1
1 National Radio Astronomy Observatory, Socorro, NM 87801, USA; 2 Nuffield Radio Asronomy Laboratories, Jodrell Bank, UK; 3 Raman Research Institute, Bangalore 560 080, India;
ABSTRACT:
We have observed the H168 alpha recombination line ( nu = 1374.6 MHz)
from the Sgri A complex using the C and D configurations of the VLA.
The angular resolution is 50"*20", the velocity resoltution
is ~21 km s-1 and the velocity coverage is +/-650 km s-1.
Relatively strong recombination line emssion is detected from the
SgrA-East and the SgrA-West region of the SgrA complex. The line emission
is spread over a velocity range of +/- 200 km s-1. Weaker emission
is also observed from the halo region surrounding the SgrA-West and SgrA-East
components. In this paper we present the results and a discussion of the
kinematics of the ionzied gas and the possible association of thermal gas
with the halo surrounding the SgrA region.
LINKS: Program, Author, anantha@aoc.nrao.edu
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Credits:
- Editors of this Volume: Angela Cotera & Heino Falcke
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File last modified on Monday 04 August 2003 [10:43 MDT].
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