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Molecular Outflows in B335 and B1

Published online by Cambridge University Press:  12 April 2016

N. Hirano ,
O. Kameya ,
T. Kasuga ,
H. Mikami ,
S. Saito ,
T. Umemoto  and
S. Yamamoto
N. Hirano
Affiliation:
Laboratory of Astronomy and Geophysics, Hitotsubashi University
O. Kameya
Affiliation:
Mizusawa Astrogeodynamics Observatory, National Astronomical Observatory
T. Kasuga
Affiliation:
Department of Instrument and Control Engineering, College of Engineering, Hosei University
H. Mikami
Affiliation:
Department of Astrophysics, Nagoya University
S. Saito
Affiliation:
Institute for Molecular Science
T. Umemoto
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory
S. Yamamoto
Affiliation:
Department of Astrophysics, Nagoya University

Extract

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We present the aperture synthesis observations of the CO molecular outflows associated with the low-mass young stellar objects embedded in B335 and Bl. We used the Nobeyama Millimeter Array and obtained the angular resolutions of 8.1” × 5.0” for B335 and 6.5” × 4.4” for B1.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 224 - 225
Copyright
Copyright © Astronomical Society of the Pacific 1994

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