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17 papers · 2 filters
Off-centred force-free neutron star magnetospheres
Jérôme Pétri
Neutron star electromagnetic activity produces pairs that fill their magnetosphere represented to the zeroth order by the force-free approximation. Neither dissipation nor accelera…
Spectral and polarization properties of black hole accretion disc emission: including absorption effects
Roberto Taverna, Lorenzo Marra, Stefano Bianchi +5
The study of radiation emitted from black hole accretion discs represents a crucial way to understand the main physical properties of these sources, and in particular the black hol…
The ultraluminous X-ray source bubble in NGC 5585
Roberto Soria, Manfred Pakull, Christian Motch +4
Some ultraluminous X-ray sources (ULXs) are surrounded by collisionally ionized bubbles, larger and more energetic than supernova remnants: they are evidence of the powerful outflo…
Frequency resolved radio and high-energy emission of pulsars
Quentin Giraud, Jérôme Pétri
Context. Pulsars are detected as broadband electromagnetic emitters from the radio wavelength up to high and very high energy in the MeV/GeV and sometimes even in the TeV range. Mu…
Constraining millisecond pulsar geometry using time-aligned radio and gamma-ray pulse profile
O. Benli, J. Petri, Dipanjan Mitra
Since the launch of the Fermi Gamma-Ray Space Telescope, several hundred gamma-ray pulsars have been discovered, some being radio-loud and some radio-quiet with time-aligned radio…
New Optically Identified Supernova Remnants in the Large Magellanic Cloud
Miranda Yew, Miroslav D. Filipović, Milorad Stupar +20
We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC). These objects were originally selected usi…