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5.16. CO mapping of barred spiral galaxies

Published online by Cambridge University Press:  25 May 2016

N. Kuno ,
N. Nakai ,
K. Nishiyama ,
K. Sorai ,
T. Handa  and
T. Iga
N. Kuno
Affiliation:
Nobeyama Radio Observatory, Minamimaki-mura, Minamisaku-gun, Nagano 384-13
N. Nakai
Affiliation:
Nobeyama Radio Observatory, Minamimaki-mura, Minamisaku-gun, Nagano 384-13
K. Nishiyama
Affiliation:
Nobeyama Radio Observatory, Minamimaki-mura, Minamisaku-gun, Nagano 384-13
K. Sorai
Affiliation:
Nobeyama Radio Observatory, Minamimaki-mura, Minamisaku-gun, Nagano 384-13
T. Handa
Affiliation:
Inst. of Astronomy, Univ. of Tokyo, Osawa, Mitaka, Tokyo 181
T. Iga
Affiliation:
Shinsyu Univ., Asahi, Matsumoto, Nagano 390

Extract

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We have made CO mapping observations of nearby barred spiral galaxies (NGC253, NGC3504, NGC4303, NGC4321, NGC6951, M83) with the Nobeyama 45-m telescope using the 2×2 SIS focal-plane array receiver. The purpose of this project is to investigate distribution and kinematics of molecular gas in barred spiral galaxies and the relation between star formation and them. We present some of the results (NGC3504 and NGC6951).

Type
Part II. Nuclear Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 243 - 244
Copyright
Copyright © Kluwer 1998 

References

Athanassoula, E. 1992, MNRAS 259, 345.Google Scholar
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