A BIPOLAR OUTFLOW OF IONIZED-GAS IN K3-50A - H76-ALPHA RADIO RECOMBINATION LINE AND CONTINUUM OBSERVATIONS OF K3-50

Citation
Cg. Depree et al., A BIPOLAR OUTFLOW OF IONIZED-GAS IN K3-50A - H76-ALPHA RADIO RECOMBINATION LINE AND CONTINUUM OBSERVATIONS OF K3-50, The Astrophysical journal, 428(2), 1994, pp. 670-679
Citations number
30
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
428
Issue
2
Year of publication
1994
Part
1
Pages
670 - 679
Database
ISI
SICI code
0004-637X(1994)428:2<670:ABOOII>2.0.ZU;2-B
Abstract
The H II regions near K3-50 (G70.3 + 1.6) have been imaged at high ang ular resolution (approximately 1.3'') in the continuum and the recombi nation lines H76alpha and He76alpha using the Very Large Array (VLA). The helium line is detected in only the brightest component K3-50A whi le the hydrogen line is detected in three components (K3-50A, B and C1 ). K3-50A shows a pronounced velocity gradient of approximately 150 km s-1 pc-1 along its major axis (P.A. = 160-degrees); in addition a wid e range of line widths are observed, from 20 km s-1 to 65 km s-1. Kine matics from the line data and the morphology of the continuum emission suggest that the ionized material associated with K3-50A is undergoin g a high-velocity bipolar outflow.