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A Wideband OH Emission Source

Published online by Cambridge University Press:  25 April 2016

R. N. Manchester ,
W. M. Goss  and
B. J. Robinson
R. N. Manchester
Affiliation:
Division of Radiophysics, CSIRO, Sydney
W. M. Goss
Affiliation:
Division of Radiophysics, CSIRO, Sydney
B. J. Robinson
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Observations of galactic HII regions in the longitude range 280° to 300° have recently been made at the OH-line frequencies 1612.231, 1665.402 and 1667.358 MHz using the Parkes radio telescope. Strong emission was observed at 1612 and 1665 MHz from a source near the regions of Hα emission RCW 48 and RCW 49 (Rodgers, Campbell and Whiteoak).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 212 - 214
Copyright
Copyright © Astronomical Society of Australia 1969

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References

1 Rodgers, A. W., Campbell, C. T. and Whiteoak, J. B., Mon. Not. Roy. Astr. Soc, 121, 103 (1960).Google Scholar
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