p { margin-bottom: 0.21cm; } Investigating the influence of magnetospheric pulsar winds at different pulsar evolutionary stages on their surroundings
2011/01/N/ST9/00485
Keywords
Descriptors
- ST9_11: Astrofizyka wysokich energii - promieniowanie rentgenowskie i gamma, promienie kosmiczne, neutrina
- 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 1 – announced on 2011-03-15
- Amount awarded
- 52 455 PLN
- Project start date
- 2011-12-13
- Project end date
- 2013-03-12
- Project duration
- 15 months (the same as in the proposal)
- Project status
- Project settled
Information in the final report
Publication in academic press/journals (1)
-
Numerical modelling of gamma-ray emission produced by electrons originating from the magnetospheres of millisecond pulsars in globular clusters
- Authors:
- A. Zajczyk, W. Bednarek, B. Rudak
- Academic press:
- Monthly Notices of the Royal Astronomical Society (year: 2013, volume: 432, 4, pages: 4362-3473), Publisher: Oxford University Press
- Status:
- Published
- DOI:
- 10.1093/mnras/stt704 – link to the publication