Millisecond pulsars are very fast rotating (over one hundred revolutions per second) neutron stars – a … more Formation of millisecond pulsars»
The inauguration of the H.E.S.S. II telescope took place on the HESS site in Namibia … more H.E.S.S. II Inauguration»
In the recent paper 'MOCCA code for star cluster simulations - I. Blue Stragglers, … more MOCCA code ready for detail simulations of the real size physical star clusters»
Merging compact binaries have provided the strongest motivation yet to build wide-band interferometric gravitational wave detectors. … more Cygnus X-3: a Galactic double black hole or black hole-neutron star progenitor»
The AstroGrid-PL domain grid is being built as part of the PLGrid Plus project, financed by … more AstroGrid-PL»
Telescop H.E.S.S. II has been inaugurated on July 26 2012. Built in Namibia telescope is deditated … more H.E.S.S. II First Light»
Synchrotron radiation from relativistic jets in active galactic nuclei is linearly polarized. It is evidence … more Polarization of synchrotron emission from relativistic reconfinement shocks with ordered magnetic fields»
Low mass stars (less massive then the Sun) of spectral type K and M are the … more Orbital and physical parameters of eclipsing binaries from the ASAS catalogue - IV. A 0.61 + 0.45 M_sun binary in a multiple system »
Fall 2012Prof. dr hab. Józef I. Smak - NCAC PAS, WarsawLecture plan
Penrose suggested in 1969 a possibility of extracting the rotational energy of a black hole … more Collisional Penrose process near the horizon of extreme Kerr black holes»