activity
19952005
most citedConstraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass

78 citations · 82 across the 5 of their papers we have counts for

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astro-ph200578 cited

Constraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass

M. Bejger, T. Bulik, P. Haensel

The moment of inertia of the pulsar A in the neutron star binary J0737-3039 will soon be measurable through detailed measurements of the periastron advance. We present the calculat…

astro-ph2003

Compact object mergers as progenitors of short bursts

T. Bulik, K. Belczynski

Compact object mergers are possible progenitors of short bursts. We analyze properties of compact object mergers using the StarTrack population synthesis code, and find that the do…

astro-ph20022 cited

On Radiation Drag and Neutrons in GRBs

Tomasz Bulik, Marek Sikora, Rafal Moderski

As it was recently shown by Derishev etal (1999), initial GRB ejecta are likely to contain comparable number of protons and neutrons. During acceleration process, and/or later, due…

astro-ph20021 cited

High-energy radiation from pulsars: a challenge to polar-cap models

B. Rudak, J. Dyks, T. Bulik

Spectacular results of pulsar observations in X-ray and gamma-ray domains gave a new boost to theoretical models of pulsar magnetospheric activity. A challenging aspect of these ef…

astro-ph20021 cited

The dependence of observed gamma-ray pulsar spectra on viewing geometry

Agnieszka Wozna, Jaroslaw Dyks, Tomasz Bulik +1

We calculate the gamma-ray lightcurves and spectra of rotation powered pulsars for a wide range of observer's viewing angles, and inclination angles of the magnetic axis to the rot…

astro-ph2002

Population synthesis of compact objects: neutron stars, strange (quark) stars and black holes

Krzysztof Belczynski, Tomasz Bulik, Wlodzimierz Kluzniak

We compute and present the distribution in mass of single and binary neutron stars, strange stars, and black holes. The calculations were performed using a stellar population synth…