Relativistic radiative magnetohydrodynamical simulations of accretion disks in black hole binaries: implications for black hole transients.
2018/29/N/ST9/02139
Keywords
Descriptors
- ST9_12: Astrofizyka relatywistyczna - procesy wokół obiektów zwartych (białych karłów, gwiazd neutronowych i czarnych dziur)
Panel
ST9 – Astronomy and space science: astrophysics, astrochemistry, astrobiology, solar system, planetary systems, stellar, galactic and extragalactic astronomy, space science, instrumentation
Host institution
Centrum Astronomiczne im. Mikołaja Kopernika PAN
Voivodeship: mazowieckie
Principal investigator (from the host institution)
Number of co-investigators in the project: 2
Call
PRELUDIUM 15 – announced on 2018-03-15
- Amount awarded
- 89 880 PLN
- Project start date
- 2019-03-15
- Project end date
- 2021-03-14
- Project duration
- 24 months (the same as in the proposal)
- Project status
- Project settled
Project description
Download the project description in a pdf file
Note — project descriptions were prepared by the authors of the applications themselves and placed in the system in an unchanged form.
Information in the final report
Publication in academic press/journals (1)
-
Looking for the underlying cause of black hole X-ray variability in GRMHD simulations
- Authors:
- D. A. Bollimpalli, R. Mahmoud, C. Done , P. C. Fragile, W. Kluźniak, , R. Narayan, C. White
- Academic press:
- Monthly Notices of the Royal Astronomical Society (year: 2020, volume: 496, pages: 20), Publisher: Oxford University Press
- Status:
- Published
- DOI:
- 10.1093/mnras/staa1808 – link to the publication