742 citations · 762 across the 7 of their papers we have counts for
7 papers
Statistical analysis of kicked black holes from TNG300 simulation
Majda Smole, Miroslav Micic
Asymmetric emission of gravitational waves during mergers of black holes (BHs) produces a recoil kick, which can set a newly formed BH on a bound orbit around the center of its hos…
Spatial field reconstruction with INLA: Application to simulated galaxies
Majda Smole, João Rino-Silvestre, Santiago González-Gaitán +1
Aims. Monte Carlo Radiative Transfer (MCRT) simulations are a powerful tool for understanding the role of dust in astrophysical systems and its influence on observations. However,…
EmulART: Emulating Radiative Transfer -- A pilot study on autoencoder based dimensionality reduction for radiative transfer models
João Rino-Silvestre, Santiago González-Gaitán, Marko Stalevski +4
Dust is a major component of the interstellar medium. Through scattering, absorption and thermal re-emission, it can profoundly alter astrophysical observations. Models for dust co…
Recoiling supermassive black holes in analytical and numerical galaxy potential
Majda Smole, Miroslav Micic, Ana Mitrašinović
We follow trajectories of recoiling supermassive black holes (SMBHs) in analytical and numerical models of galaxy merger remnants with masses of and $10^{12}…
Black holes, gravitational waves and fundamental physics: a roadmap
Leor Barack, Vitor Cardoso, Samaya Nissanke +203
The grand challenges of contemporary fundamental physics---dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem-…
SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
Majda Smole, Miroslav Micic, Nemanja Martinovic
We make black hole (BH) merger trees from Millennium and Millennium-II simulations to find under what conditions 10^9Msun SMBH can form by redshift z=7. In order to exploit both: l…
Detection of a 1.59 h period in the B supergiant star HD 202850
Michaela Kraus, Sanja Tomic, Mary E. Oksala +1
Photospheric lines of B-type supergiants show variability in their profile shapes. In addition, their widths are much wider than can be accounted for purely by stellar rotation. Th…