Direct probe of the inner accretion flow around the supermassive black hole in NGC 2617

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484708" target="_blank" >RIV/67985815:_____/17:00484708 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201628686" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201628686</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201628686" target="_blank" >10.1051/0004-6361/201628686</a>

Result language
angličtina
Original language name
Direct probe of the inner accretion flow around the supermassive black hole in NGC 2617
Original language description
NGC2617 is a nearby (z similar to 0 : 01) active galaxy that recently switched from being a Seyfert 1.8 to be a Seyfert 1.0. At the same time, it underwent a strong increase of X-ray flux by one order of magnitude with respect to archival measurements. We characterise the X-ray spectral and timing properties of NGC2617 with the aim of studying the physics of a changing-look active galactic nucleus (AGN).nWe performed a comprehensive timing and spectral analysis of two XMM-Newton pointed observations spaced by one month, complemented by archival quasi-simultaneous INTEGRAL observations.
Czech name
—
Czech description
—

Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)