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Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background

Detalles Bibliográficos
Autores principales: Yi, I, Boughn, S P
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:http://cds.cern.ch/record/347677
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author Yi, I
Boughn, S P
author_facet Yi, I
Boughn, S P
author_sort Yi, I
collection CERN
id cern-347677
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1998
record_format invenio
spelling cern-3476772019-09-30T06:29:59Zhttp://cds.cern.ch/record/347677engYi, IBoughn, S PRadio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray backgroundAstrophysics and AstronomyIASSNS-AST-98-6oai:cds.cern.ch:3476771998
spellingShingle Astrophysics and Astronomy
Yi, I
Boughn, S P
Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title_full Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title_fullStr Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title_full_unstemmed Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title_short Radio/X-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the X-ray background
title_sort radio/x-ray luminosity relation for advection-dominated accretion: implications for emission line galaxies and the x-ray background
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/347677
work_keys_str_mv AT yii radioxrayluminosityrelationforadvectiondominatedaccretionimplicationsforemissionlinegalaxiesandthexraybackground
AT boughnsp radioxrayluminosityrelationforadvectiondominatedaccretionimplicationsforemissionlinegalaxiesandthexraybackground