FERO: Finding extreme relativistic objects - I. Statistics of relativistic Fe K? lines in radio-quiet Type 1 AGN

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00352724" target="_blank" >RIV/67985815:_____/10:00352724 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

FERO: Finding extreme relativistic objects - I. Statistics of relativistic Fe K? lines in radio-quiet Type 1 AGN

Original language description

Accretion models predict that fluorescence lines broadened by relativistic effects should arise from reflection of X-ray emission onto the inner region of the accretion disc surrounding the central black hole of active galactic nuclei (AGN). The theory behind the origin of relativistic lines is well established, and observational evidence from a moderate number of sources seems to support the existence of these lines. The aim of this work is to establish the fraction of AGN with relativistic Fe K? lines, and study possible correlations with source physical properties.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2010

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy and Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

524

Issue of the periodical within the volume

Dec

Country of publishing house

FR - FRANCE

Number of pages

22

Pages from-to

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UT code for WoS article

000284625300017

EID of the result in the Scopus database

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