Scintillation-induced variability in radio absorption spectra against extragalactic sources

Spectral features absorbed against some radio quasars exhibit ~50 mJy variations, with the lines varying both relative to the continuum and, when several lines are present, even relative to one another. We point out that such variability can be expected as a consequence of refractive scintillation c...

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Main Author: Macquart, Jean-pierre
Format: Journal Article
Published: EDP Sciences 2005
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/40033
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author Macquart, Jean-pierre
author_facet Macquart, Jean-pierre
author_sort Macquart, Jean-pierre
building Curtin Institutional Repository
collection Online Access
description Spectral features absorbed against some radio quasars exhibit ~50 mJy variations, with the lines varying both relative to the continuum and, when several lines are present, even relative to one another. We point out that such variability can be expected as a consequence of refractive scintillation caused by the interstellar medium of our Galaxy. Scintillation can cause independent variations between closely-spaced spectral lines, and can even alter the line profile. The background source need not he compact to exhibit spectral variability. The variability can he used to infer the parsec to sub-parsec scale structure of the intervening absorbing material. We discuss the importance of scintillation relative to other possible origins of spectral variability. The present theory is applied to account for the variations observed in the HI-absorbed quasar PKS I 127-145.
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publishDate 2005
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spelling curtin-20.500.11937-400332017-09-13T15:53:17Z Scintillation-induced variability in radio absorption spectra against extragalactic sources Macquart, Jean-pierre Interstellar matter Variability Galaxy structure Continuum scattering Galaxies Absorption spectra radio lines Line shape high angular resolution Extragalactic source Quasars Radio spectrum Spectral features absorbed against some radio quasars exhibit ~50 mJy variations, with the lines varying both relative to the continuum and, when several lines are present, even relative to one another. We point out that such variability can be expected as a consequence of refractive scintillation caused by the interstellar medium of our Galaxy. Scintillation can cause independent variations between closely-spaced spectral lines, and can even alter the line profile. The background source need not he compact to exhibit spectral variability. The variability can he used to infer the parsec to sub-parsec scale structure of the intervening absorbing material. We discuss the importance of scintillation relative to other possible origins of spectral variability. The present theory is applied to account for the variations observed in the HI-absorbed quasar PKS I 127-145. 2005 Journal Article http://hdl.handle.net/20.500.11937/40033 10.1051/0004-6361:20034425 EDP Sciences fulltext
spellingShingle Interstellar matter
Variability
Galaxy structure
Continuum
scattering
Galaxies
Absorption spectra
radio lines
Line shape
high angular resolution
Extragalactic source
Quasars
Radio spectrum
Macquart, Jean-pierre
Scintillation-induced variability in radio absorption spectra against extragalactic sources
title Scintillation-induced variability in radio absorption spectra against extragalactic sources
title_full Scintillation-induced variability in radio absorption spectra against extragalactic sources
title_fullStr Scintillation-induced variability in radio absorption spectra against extragalactic sources
title_full_unstemmed Scintillation-induced variability in radio absorption spectra against extragalactic sources
title_short Scintillation-induced variability in radio absorption spectra against extragalactic sources
title_sort scintillation-induced variability in radio absorption spectra against extragalactic sources
topic Interstellar matter
Variability
Galaxy structure
Continuum
scattering
Galaxies
Absorption spectra
radio lines
Line shape
high angular resolution
Extragalactic source
Quasars
Radio spectrum
url http://hdl.handle.net/20.500.11937/40033