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Starbursts in Clumpy Irregular Galaxies

Published online by Cambridge University Press:  03 August 2017

R. Augarde ,
M. Auriere ,
L. Bottinelli ,
G. Coupinot ,
R. Futaully ,
L. Gouguenheim  and
J. Hecquet
R. Augarde
Affiliation:
Observatoire de Marseille, 13248 Marseille Cedex 4, France
M. Auriere
Affiliation:
Observatoire du Pic du Midi, 65200 Bagnères de Bigorre, France
L. Bottinelli
Affiliation:
Observatoire de Meudon, 92195 Meudon Principal Cedex, France
G. Coupinot
Affiliation:
Observatoire du Pic du Midi, 65200 Bagnères de Bigorre, France
R. Futaully
Affiliation:
Observatoire du Pic du Midi, 65200 Bagnères de Bigorre, France
L. Gouguenheim
Affiliation:
Observatoire de Meudon, 92195 Meudon Principal Cedex, France
J. Hecquet
Affiliation:
Observatoire du Pic du Midi, 65200 Bagnères de Bigorre, France

Extract

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Bright Clumpy Irregular galaxies (CI) are characterized by intense star formation activity. At the present time, a few objects of this type is known; to search for new candidates, and to investigate the causes of this intense star formation, we observe a sample of galaxies selected mainly from Kiso Schmidt survey.

Type
II- Early-type and Irregular Galaxies
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 48
Copyright
Copyright © Kluwer 1991 

References

Krause, M., Cox, P., Garcia-Barreto, J.A., Downes, D.: 1990, Astron. Astrophys. 233, L1 Google Scholar
van der Kruit, P.C., Oort, J.H., Mathewson, D.S.: 1972, Astron. Astrophys. 21, 169 Google Scholar