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Detection of Extragalactic CH 9-cm Emission with the Nancay Radio Telescope

Published online by Cambridge University Press:  03 August 2017

L. Bottinelli
Affiliation:
Observatoire de Paris and Université Paris-Sud
L. Gouguenheim
Affiliation:
Observatoire de Paris and Université Paris-Sud
E. Gerard
Affiliation:
Observatoire de Paris
A.M. Le Squeren
Affiliation:
Observatoire de Paris
J.M. Martin
Affiliation:
Observatoire de Paris
M. Dennefeld
Affiliation:
Institut d'Astrophysique de Paris

Extract

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As part as of an extragalactic CH 9-cm ground-state emission survey of OH emitters (megamasers) and absorbers, we report the detections of the 3335 MHz main line in M82 and of the 3264 MHz satellite line in the luminous far infrared (FIR) galaxies NGC 3079 and NGC 5793, obtained with the Nançay radiotelescope.

Type
VI- Other Gaseous Components
Copyright
Copyright © Kluwer 1991 

References

Bouloy, D, Nguyen-Quang-Rieu, , Field, D: 1984, Astron. Astrophys. 130, 380 Google Scholar
Bujarrabal, V., Gonzalo, I., Salinas, F.: 1984, Ap. J. 285, 312 Google Scholar
Martin, J.M., Bottinelli, L., Dennefeld, M., Gouguenheim, L., Le Squeren, A.M.: 1988, Astron. Astrophys. 201, L15 Google Scholar