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The Molecular Spiral Structure in M51 Derived from CO(J=2-1) Line Observations

Published online by Cambridge University Press:  14 August 2015

M. Guélin ,
S. Garcia-Burillo ,
R. Blundell ,
J. Cernicharo ,
D. Despois  and
H. Steppe
M. Guélin
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain
S. Garcia-Burillo
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain
R. Blundell
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain
J. Cernicharo
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain
D. Despois
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain
H. Steppe
Affiliation:
IRAM, Domaine Universitaire, 38406 Saint Martin d’Hères, France and Avenida Divina Pastora 7, 18012 Granada, Spain

Abstract

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We present preliminary results of a high angular resolution-high sensitivity survey of CO(J = 2—1) line emission in M51 made with the IRAM 30 m telescope.

Type
Joint Commission Meeting
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 575 - 577
Copyright
Copyright © Kluwer 1989

References

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