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Carbon Recombination Lines at 34.5 MHz from the Galactic Plane

Published online by Cambridge University Press:  26 May 2016

N.G. Kantharia  and
K.R. Anantharamaiah
N.G. Kantharia
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune, India
K.R. Anantharamaiah
Affiliation:
Raman Research Institute, Sadashivnagar, Bangalore, India

Abstract

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We report the detection of carbon radio recombination lines (CRRLs) near 34.5 MHz (n ∼ 575) and near 328 MHz (n ∼ 270) from 6 positions with l < 17°, b = 0°. Modelling the data shows that the observed CRRLs can arise under a range of physical conditions which are found in atomic HI, molecular and photo-dissociation regions (PDRs) in the galactic disk.

Type
Part 6: Spectral Studies of our Galaxy
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 347 - 348
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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