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BHmapping SIGNED

Mapping the inner flow around accreting black holes

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 BHmapping project word cloud

Explore the words cloud of the BHmapping project. It provides you a very rough idea of what is the project "BHmapping" about.

issue    regarding    group    center    close    source    theoretical    hotly    geometry    science    behaviours    inflowing    mechanism    accretion    cross    bh    regions    environments    function    models    flow    gas    biggest    variations    data    coupling    bhs    linked    competitive    spectral    black    relevance    temporal    distances    nature    possibility    strictly    astrophysical    launch    extend    ray    flux    spin    emitting    location    nicolaus    understanding    innovative    pioneered    copernicus    techniques    expertise    tightly    payload    timing    vicinity    binaries    quality    academy    er    galactic    astrosat    responsible    modern    candidate    astronomy    reverberation    nuclei    emerge    astronomical    relativity    researcher    constrained    skills    map    polish    nicer    supermassive    central    satellite    accreting    accreted    renowned    disputed    unsolved    astrophysics    fundamental    active    observational    energy    geometrical    jet    holes   

Project "BHmapping" data sheet

The following table provides information about the project.

Coordinator
CENTRUM ASTRONOMICZNE IM. MIKOLAJAKOPERNIKA POLSKIEJ AKADEMII NAUK 

Organization address
address: Bartycka, 18
city: WARSZAWA
postcode: 716
website: http://www.camk.edu.pl

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Poland [PL]
 Total cost 134˙462 €
 EC max contribution 134˙462 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2017
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2019
 Duration (year-month-day) from 2019-02-01   to  2021-01-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    CENTRUM ASTRONOMICZNE IM. MIKOLAJAKOPERNIKA POLSKIEJ AKADEMII NAUK PL (WARSZAWA) coordinator 134˙462.00

Map

 Project objective

Understanding the behaviour of matter in the close environments of astrophysical black holes (BH) is one of the biggest challenges of modern astrophysics. This project aims to address the fundamental problem of determining the geometry of the inflowing matter around accreting BHs. The geometrical distribution of the accreted gas is a hotly disputed and still unsolved issue. Its relevance is tightly linked to the possibility of testing the effects of General Relativity in the vicinity of BHs. Moreover, it is strictly related to other fundamental problems, in particular regarding the nature and location of the X-ray source, the mechanism responsible for the launch of the jet and the determination of the BH spin. We propose to use a novel approach known as “X-ray reverberation”. This is based on the use of innovative cross-spectral-timing techniques to study the temporal response of the accreting gas to flux variations of the central X-ray source, thus allowing distances among the different emitting regions to be constrained. This project will use the best quality data, including those provided by the ASTROSAT satellite and the NICER payload. We aim to: map the evolving geometry of the accretion flow as a function of accretion state in Galactic BH X-ray binaries; study the coupling between the accretion flow and the jet; develop theoretical spectral-timing models to explain the data; investigate how these behaviours extend to the supermassive BHs in active galactic nuclei. The candidate is an experienced researcher (ER) in the field of observational X-ray astronomy, and has pioneered the application of the X-ray reverberation method to several accreting BH systems. By exploiting the long-term and renowned expertise in theoretical modelling of accretion processes around BHs of the High Energy Astrophysics group at the Nicolaus Copernicus Astronomical Center of the Polish Academy of Science, this research will allow the ER to emerge with new and competitive skills.

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The information about "BHMAPPING" are provided by the European Opendata Portal: CORDIS opendata.

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