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Observations of H2O maser and continuum emission in AFGL 2591

Published online by Cambridge University Press:  03 August 2017

Miguel A. Trinidad
Affiliation:
Instituto de Astronomía, (UNAM), Apdo. Postal 70-264, D.F. 04510, México
Salvador Curiel
Affiliation:
Instituto de Astronomía, (UNAM), Apdo. Postal 70-264, D.F. 04510, México
Jorge Cantó
Affiliation:
Instituto de Astronomía, (UNAM), Apdo. Postal 70-264, D.F. 04510, México
José M. Torrelles
Affiliation:
Institut d'Estudis Espacials de Catalunya (IEEC/CSIC) and Instituto de Ciencias del Espacio (CSIC), Edifici Nexus, C/ Gran Capità, 2-4, E-08034 Barcelona, Spain
Luis F. Rodríguez
Affiliation:
Instituto de Astronomía, (UNAM), Apdo. Postal 3-72 (Xangari) 58089 Morelia, Michoacán, México
José F. Gómez
Affiliation:
Laboratorio de Astrofísica Espacial y Física Fundamental (INTA), Apdo. Correos 50727, E-28080 Madrid, Spain
Paul T.P. Ho
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138

Abstract

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We report results of radio continuum (1.3 and 3.6 cm) and H2O maser line observations, made with the Very Large Array (A configuration), toward the star-forming region AFGL 2591. We detected 85 maser spots toward this region, which are distributed in three main groups. Two of these groups spatially coincide with the radio continuum sources VLA 2 and VLA 3. The maser spots associated with VLA 3 are distributed along a shell-like structure of 0.01 and nearly perpendicular to the CO bipolar outflow. We propose that VLA 3 is the center of the observed molecular flow in this region. Finally, we confirm that AFGL 2591 region is a cluster of B type stars, each one with its own optically thin H II region.

Type
Part 1. Star Formation
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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