Warm absorber and truncated accretion disc in IRAS 05078+1626

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00345820" target="_blank" >RIV/67985815:_____/10:00345820 - 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

Warm absorber and truncated accretion disc in IRAS 05078+1626

Original language description

We investigate the central environment of a Seyfert 1.5 galaxy IRAS 05078+1626 with the EPIC and RGS instruments onboard XMM-Newton. Our study represents the first X-ray spectroscopic measurement of this galaxy. The spectrum unveils some of the standardingredients in Seyfert galaxies, such as a power law primary continuum, modified by reflection from the accretion disc and by the effect of complex, multi-phase obscuration. However, data constrains the accretion disc, if present, not to extend closer than to 60 gravitational radii from the black hole.

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

Result was created during the realization of more than one project. More information in the Projects tab.

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

512

Issue of the periodical within the volume

Mar-Apr

Country of publishing house

FR - FRANCE

Number of pages

8

Pages from-to

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UT code for WoS article

000276245500029

EID of the result in the Scopus database

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