Grant: Discovery Grants Program - Individual
Saint Mary's University
$27,000.00
The innermost environment of young supermassive black holes
EF 2013-14
Résumé
How does material fall into a black hole? What is the material falling into a black hole made of? How close does it get to the black hole before it disappears? Do black holes spin? We live in a unique era in that we can now attempt to answer such questions based on observations, and not theory alone. X-rays are emitted from the regions closest to black holes, where temperatures and conditions are most extreme. By studying the X-ray variability and spectral properties of supermassive black holes, known as active galactic nuclei, we can decipher what the environment nearest the black hole looks like. The proposed plan is to observe active galaxies with deep X-rays observations at various epochs over the course of years. Characterising the behaviour of the black holes on short (e.g. hourly) and long (e.g. month-years) time scales will reveal their intrinsic properties.
Programme
Discovery Grants Program - Individual
Bénéficiaire
Emplacement
Nova Scotia, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
355157-2010
Name nom
Gallo, Luigi
Department département
Astronomy and Physics
Organization id
85
Institution établissement
Saint Mary's University
Province en
Nova Scotia
Province fr
Nouvelle-Écosse
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2013
Competition year année de concours
2010
Award amount
27000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
Area of application code
1202
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Physical sciences
Area of application fr
Sciences physiques
Research subject code
3200
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Astronomy and astrophysics
Research subject fr
Astronomie et astrophysique
Partie
4
Nb partie
5
Application title
The innermost environment of young supermassive black holes
Keyword
NSERC
Application summary
How does material fall into a black hole? What is the material falling into a black hole made of? How close does it get to the black hole before it disappears? Do black holes spin? We live in a unique era in that we can now attempt to answer such questions based on observations, and not theory alone. X-rays are emitted from the regions closest to black holes, where temperatures and conditions are most extreme. By studying the X-ray variability and spectral properties of supermassive black holes, known as active galactic nuclei, we can decipher what the environment nearest the black hole looks like. The proposed plan is to observe active galaxies with deep X-rays observations at various epochs over the course of years. Characterising the behaviour of the black holes on short (e.g. hourly) and long (e.g. month-years) time scales will reveal their intrinsic properties.