Our Research

The fourth division (BP4) of The Fundamental Research Department (Departament Badań Podstawowych) deals with research in astrophysics and astronomy, mainly their observational aspects. The BP4 division is located in Warsaw at 7 Pasteura street.

The research conducted at the Astrophysics Laboratory includes:

  • Cosmology: CMB, large structures of the Universe, dark matter, non-standard cosmology and gravitational lensing
  • Gravitational waves: Multi-messenger astronomy, new tools for cosmology
  • Physics of galaxies: Formation and evolution of galaxies, AGN, quasars and gamma-ray burst
  • Interstellar medium: Star formation, neutron stars and white dwarfs
Check our Research Fields page for more information.


The BP4 division is also involved in several international projects. Check our Scientific Projects page for more information.

 

Seminars

Upcoming seminars for all of NCBJ can be found here.

The seminar archive for NCBJ can be found here.

 

Latest News

Scroll down for the latest news about the research done by our division or click here.

Conference Participation

BP4 participate in may national and intersectional conferences. We share our cutting edge research and enthusiasm with other astronomers across the world. Below are pictures from our trips across the globe.

Latest News

Professor Agnieszka Pollo has taken the position of Deputy Director for Science at NCBJ

On October 16, 2023, a change took place in the position of Deputy Director for Science at NCBJ. The former director, Professor Ewa Rondio, passed on her duties to Professor Agnieszka Pollo, an astrophysicist who has been successfully leading the rapidly developing Department of Astrophysics.

Zdjęcie: Artystyczna interpretacja odpływów galaktycznych. Aktywność gwiazdotwórcza może skutkować powstawaniem potężnych wiatrów (odpływów), które są w stanie przenosić gaz na bardzo duże odległości, aż do przestrzeni międzygalaktycznej. Linie emisyjne [CII] 158 μm wyraźnie wskazują na odpływ gazu atomowego. Źródło: ESA/Hubble, ESO/L. Calçada, M. Romano.

Galactic outflows drive the evolution of dwarf galaxies

Stellar feedback is expected to play a key role in regulating the evolution of low-mass galaxies by producing galactic-scale winds (also known as outflows) that push the gas away from the interstellar medium, eventually preventing from the formation of new stars. In this respect, an international team of astronomers led by NCBJ scientist, have published a work on the Astronomy & Astrophysics journal addressing the impact of galactic outflows on the baryonic cycle of nearby dwarf galaxies

Stanisław Mrówczyński podczas Specjalnego Colloquium DBP (foto: Marek Pawłowski / NCBJ)

Annual Awards Presented by the Fundamental Research Department of NCBJ

On June 26, 2023, a Special Colloquium was held, during which awards were presented for the best research and popularization activities in 2022 at the Fundamental Research Department. The winners were Prof. Michał Bluj, a team consisting of Prof. Paweł Ziń and Dr. Maciej Pylak, Dr. Michael Romano, and Prof. Jerzy Kowalski-Glikman and Dr. Miguel Figueira

Zawartość gwiazdowo-pyłowa w funkcji wieku Wszechświata. Rozkład osiąga szczyt w okolicach kosmicznego południa.

Unveiling the hidden stars: ALMA Shines a Light on Dust Attenuation

Interstellar dust is a key component in galaxies. It favors star formation and drives the chemistry and physics of the interstellar medium. However, it hides the majority of stars in a way that it is impossible to observe them. Astrophysicists use dust attenuation laws that would uncover these hidden stars by reverse-engineering the light from galaxies to quantify how many stars are there.

Wizja artystyczna i zdjęcie rentgenowskie galaktyki MRK 1216 typu "red nugget". Źródło: X-ray: NASA/CXC/MTA-Eötvös University/N. Werner et al., Ilustracja: NASA/CXC/M. Weiss

The project of a PhD student of the NCBJ Department of Astrophysics qualified for the „Pearls of Science” program

The first edition of the competition under the „Pearls of Science” program has been settled. One of the scientists qualified for the program is Krzysztof Lisiecki, MSc, a PhD student at the Astrophysics Department of the National Center for Nuclear Research, conducting research in the project „In search of witnesses to the early Universe – studying the properties of red nuggets”.

Zdjęcie z przeglądu H20/Cosmic Dawn wybrane przez użytkownika Galaxy Zoo Talk graham_d

New images of tens of thousands of galaxies have been made available at the Galactic Zoo

Twenty thousand high quality images from the Hawaii Two-0 (H20)/Cosmic Dawn survey have been released to the public on the most popular citizen science project: Galaxy Zoo. Anyone in the world can become a citizen scientist and help astronomers classify images from the Subaru telescope.