An international team of astronomers, including Rodolfo Smiljanic from the Nicolaus Copernicus Astronomical Center in Warsaw, have … more Four stars on the way to become a type Ia supernova»
Despite the unclear situation with the COVID pandemic the Nicolaus Copernicus Astronomical Center will organize the summer … more Summer Student Program 2022»
A team of astronomers, including Jean-Pierre Lasota from the Copernicus Astronomical Center in Warsaw, with the … more Micronovae, a new kind of stellar explosion»
The Cassegrain U-Band Efficient Spectrograph (CUBES) is a new instrument being built for the 8-meter … more Simulated observations with the CUBES spectrograph»
Przedmiotem postępowania jest DOSTAWA GEOFONÓW ORAZ DWÓCH SEJSMOMETRÓW SZEROKOPASMOWYCH WRAZ Z DWOMA REJESTRATORAMI DANYCH POMIAROWYCH. Zapraszamy do … more DOSTAWA GEOFONÓW ORAZ DWÓCH SEJSMOMETRÓW SZEROKOPASMOWYCH WRAZ Z DWOMA REJESTRATORAMI DANYCH POMIAROWYCH»
Neutron stars are superfluid. This is good news for theoretical physicists: they have an excuse to … more Neutron star superfluid-viscous hydrodynamics»
Neutron stars, although very strongly bound by gravity, may be deformed due to the rapid rotation … more Gravitational darkening effect on the spectrum of a hot, rapidly rotating neutron star»
The article "A search for cool molecular gas in GK Persei and other classical novae", by … more A search for cool molecular gas in GK Persei and other classical novae»
Population II Cepheids are old population pulsating stars. They are less known than famous Classical Cepheids … more An absolute calibration of the Period-Luminosity Relations for Type II Cepheids»
Symbiotic stars are one of the most active classes of binary systems. They are composed of … more SALT uncovers the nature of the jet-producing symbiotic binary St 2-22»