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Photometric, Spectroscopic and 21-cm Line Investigation of Selected UV-Excess KISO and Clumpy Galaxies

Published online by Cambridge University Press:  04 August 2017

L. Bottinelli ,
L. Gouguenheim ,
M. Hamabe ,
J. Heidmann ,
H. Maehara  and
B. Takase
L. Bottinelli
Affiliation:
Paris Observatory, Meudon 92195, France
L. Gouguenheim
Affiliation:
Paris Observatory, Meudon 92195, France
M. Hamabe
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
J. Heidmann
Affiliation:
Paris Observatory, Meudon 92195, France
H. Maehara
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
B. Takase
Affiliation:
Kokugakuin University, Shibuya, Tokyo 150, Japan

Extract

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A survey of Kiso UV-excess galaxies (KUGs) has been made using the 105-cm Kiso Schmidt telescope. We selected three galaxies of Ic-type (i.e. irregulars with clumpy HII regions). KUGs 1618+373, 1624+404 and 1626+413, and observed them together with a clumpy irregular galaxy Mrk 297 to clarify their star formation activity (Maehara et al. 1986).

Type
II. Large Scale Processes of Star Formation
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 648 - 650
Copyright
Copyright © Reidel 1987 

References

Maehara, H., Hamabe, M., Bottinelli, L., Gouguenheim, L., Heidmann, J., and Takase, B.: 1986, in preparation.Google Scholar