336 citations · 448 across the 9 of their papers we have counts for
9 papers
SAMSum Corpus: A Human-annotated Dialogue Dataset for Abstractive Summarization
Bogdan Gliwa, Iwona Mochol, Maciej Biesek +1
This paper introduces the SAMSum Corpus, a new dataset with abstractive dialogue summaries. We investigate the challenges it poses for automated summarization by testing several mo…
Pulsar striped winds
Iwona Mochol
According to magnetohydrodynamic (MHD) models, the rotational energy of a rapidly spinning neutron star is carried away by a relativistic wind and deposited at a large distance, in…
Very high energy emission as a probe of relativistic magnetic reconnection in pulsar winds
Iwona Mochol, Jerome Petri
The population of gamma-ray pulsars, including Crab observed in the TeV range, and Vela detected above 50 GeV, challenges existing models of pulsed high-energy emission. Such model…
The stability of strong waves and its implications for pulsar wind shocks
Iwona Mochol, John G. Kirk
Strong waves can mediate a shock transition between a pulsar wind and its surroundings, playing the role of an extended precursor, in which the energy is effectively transferred fr…
Radiative damping and emission signatures of strong superluminal waves in pulsar winds
Iwona Mochol, John G. Kirk
We analyse the damping by radiation reaction and by Compton drag of strong, superluminal electromagnetic waves in the context of pulsar winds. The associated radiation signature is…
High-energy emission from pulsar binaries
Iwona Mochol, John G. Kirk
Unpulsed, high-energy emission from pulsar binaries can be attributed to the interaction of a pulsar wind with that of a companion star. At the shock between the outflows, particle…
Superluminal Waves and the Structure of Pulsar Wind Termination Shocks
Iwona Mochol, John G. Kirk
The termination shock of a pulsar wind is located roughly where the ram pressure matches that of the surrounding medium. Downstream of the shock, MHD models of the diffuse nebular…
Propagation and stability of superluminal waves in pulsar winds
Iwona Mochol, John G. Kirk
Nonlinear electromagnetic waves with superluminal phase velocity can propagate in the winds around isolated pulsars, and around some pulsars in binary systems. Using a short-wavele…
Charge-starved, relativistic jets and blazar variability
John G. Kirk, Iwona Mochol
High energy emission from blazars is thought to arise in a relativistic jet launched by a supermassive black hole. The emission site must be far from the hole and the jet relativis…