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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1080

Title: Low density ionized gas in the inner Galaxy - interpretation of recombination line observations at 325 MHz.
Authors: Anantharamaiah, K.R.
Keywords: Galaxy
Recombinational lines
Galactic rige
Interstellar medium
Electron densities
H2 regions
Low density envelopes
Issue Date: 1985
Publisher: Indian Academy of Sciences, Bangalore, India.
Citation: Journal of Astrophysics and Astronomy, 1985, Vol. 6, p203-226.
Abstract: The properties of diffuse ionized gas in the inner Galaxy are derived from a recent survey of the H 272-alpha recombination line (324.99 MHz) in the direction of 34 H II regions, 12 SNRs, and six regions of continuum minimum in the Galactic plane. The derived properties of the gas are an electron density of 0.5-6/cu cm, an electron temperature of 3000-8000 K, and emission measures of 500-3000 pc/cm exp 6. It is suggested that the low-frequency recombination lines arise in low-density envelopes of the H II regions; it is found that these envelopes should have electron densities in the range 1-10/cu cm and linear sizes of 30-300 pc in order to produce the observed H 272-alpha lines.
URI: http://hdl.handle.net/2289/1080
ISSN: 0250-6335
Copyright: Indian Academy of Sciences, Bangalore, India.
Appears in Collections:Research Papers (A&A)

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