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Detecting continuous gravitational waves (GWs) from rapidly spinning, asymmetric neutron stars in our Galaxy is extremely … more Microlensing of long-duration gravitational wave signals originating from Galactic sources»
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Pulsars are rapidly rotating neutron stars, whose rotation rate can be accurately tracked with the aid … more Pulsars: continuous gravitational wave signal»
The paper Neural Posterior Estimation of Neutron Star Equations of State, by Valéria Carvalho, Márcio Ferreira, Michał Bejger … more Estimation of Neutron Star Equations of State»
WFI Consortium Meeting was helsd on 3-7 th May 2021. Again it was online meeting and … more 13th X-IFU Consortium Meeting»
This autumn as usually WFI Consortium Meeting (9-12.11.2020). It was online meeting due to circumstances and … more 12th WFI Consortium Meeting»
November 2-6, 2020 our consortium meeting was also online this time. Polish team members participated actively … more 12th X-IFU Consortium Meeting»
11th WFI Consortium Meeting was held online as well. Because of difficult pandemic situation all around … more 11th WFI Consortium Meeting»
Gas and dust flowing from stars can, under the right conditions, clash with a star’s surroundings …
The paper 
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