Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-24T15:38:39.243Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Kutner, M. L., Leous, J., and Verter, F., 1990, (in preparation).Google Scholar
Kutner, M. L., Verter, F., and Rickard, L. J, 1990, Astrophys. J., 10 Dec.Google Scholar
Pellet, A., Astier, N., Viale, A., Courtes, G., Maucherat, A., Monnet, G., and Walterbos, R. A. M., and Schwering, P. B. W., 1987, A. & A., 180, 287.Google Scholar
Welch, , et al. 1986, Astrophys. J., 305, 586.Google Scholar