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A New Technique for Measuring Impact‐broadened Radio Recombination Lines in HiiRegions: Confrontation with Theory at High Principal Quantum Numbers
New, low‐noise receivers have allowed detection, in several giant Hiiregions, of Rydberg‐Rydberg transitions of hydrogen that cover a large range of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepac...
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Published in: | Publications of the Astronomical Society of the Pacific 2000-09, Vol.112 (775), p.1236-1242 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
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Summary: | New, low‐noise receivers have allowed detection, in several giant Hiiregions, of Rydberg‐Rydberg transitions of hydrogen that cover a large range of
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‐values in a single observing window. This, in turn, allows lines covering a large range in principal quantum numbernto be detected simultaneously with the same antenna beam. We have employed a new frequency‐switching technique which allows a very precise determination of the line widths. We have used this technique with the NRAO 140 foot telescope to observe lines in W51 and Orion A near 6 GHz, with
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‐values that vary by a factor of ∼21 (
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–∼21) and correspondingn‐values that vary by a factor of 2.7 (
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ISSN: | 0004-6280 1538-3873 |
DOI: | 10.1086/316611 |