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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.

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

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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