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CO(J=2 → 1) Study of Molecular Clouds in the SW Arm of M31

Published online by Cambridge University Press:  03 August 2017

M. L. Kutner ,
F. Verter  and
L. J Rickard
M. L. Kutner
Affiliation:
Physics Dept., Rensselaer Polytechnic Institute Troy, NY, USA
F. Verter
Affiliation:
NASA Goddard Spaceflight Center Greenbelt, MD, USA
L. J Rickard
Affiliation:
Naval Research Laboratory Washington, DC, USA

Abstract

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We present a map of a 3′ × 3′ section of the southwest arm of M31 in the CO(J=2 → 1) transition. We have detected emission in 25 positions out of 31 observed in a field centered at (—42.5′, +7.5) (major axis, minor axis). The map is sampled at intervals of one beamwidth, with an angular resolution of 30″ or 100 × 460 pc.

Type
I- Local Group Galaxies
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 29 - 31
Copyright
Copyright © Kluwer 1991 

References

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