A Survey of Radio Recombination Lines Using the Ooty Radio Telescope at 328 MHz in the Inner Galaxy

Details A Survey of Radio Recombination Lines Using the Ooty Radio Telescope at 328 MHz in the Inner Galaxy A Survey of Radio Recombination Lines Using the Ooty Radio Telescope at 328 MHz in the Inner Galaxy

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aj....143...26b&link_type=abstract

The Astronomical Journal, Volume 143, Issue 2, article id. 26 (2012).

Astronomy and Astrophysics

Astronomy

H Ii Regions, Ism: Abundances, Radio Lines: Ism

Scientific paper

A survey of radio recombination lines in the Galactic plane with longitude -32° < l < +80° and latitude b < ±3° using Ooty Radio Telescope (ORT) at 328 MHz is reported. ORT observations were made using a New Digital Backend (NDB) recently added to the telescope. With the NDB ORT had a beam of 2fdg3 × 2fdg2 sec(δ) and a passband of ~1 MHz in the spectral line mode. The above-mentioned Galactic region was divided into ~2° × 2° patches with the ORT beam pointed to the center. The ORT observations form a study of the distribution of extended low-density warm-ionized medium (ELDWIM) in the inner Galaxy using H271α RLs. By obtaining kinematical distances using V LSR of the H271α RLs, the distribution of ELDWIM clouds within the inner Galaxy has been deduced for the region given above.

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