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3.27. Millimeter-wave continuum observation of galaxies

Published online by Cambridge University Press:  25 May 2016

H. Matsuo ,
N. Kuno ,
B. Vila-Vilaro ,
H. Kashihara  and
T. Kawabata
H. Matsuo
Affiliation:
Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-13, Japan
N. Kuno
Affiliation:
Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-13, Japan
B. Vila-Vilaro
Affiliation:
Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-13, Japan
H. Kashihara
Affiliation:
Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-13, Japan
T. Kawabata
Affiliation:
Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-13, Japan

Extract

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Continuum observation of galaxies in millimeter-wave gives informations on dust emission from molecular clouds, free-free emission from HII region and synchrotron emission from SNR and diffuse component. The free-free emission can be observed only at millimeter-wave frequencies and their emission is optically thin, it can be a good indicator of their star-formation activities.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 143 - 144
Copyright
Copyright © Kluwer 1998 

References

Kuno, N. and Matsuo, H. (1997) Two-Millimeter Observation of the Starburst Galaxy M82, Pub. Astron. Soc. Japan, 49, pp. 265–269.CrossRefGoogle Scholar
Kuno, N., Matsuo, H., Mizumoto, Y., Lange, A.E., Beeman, J.W. and Haller, E.E. (1993) Seven Matched Bolometers for Millimeter Wave Observations, Int. J. of Infrared and Millimeter Waves, 14, pp. 749–762.CrossRefGoogle Scholar