activity
20182026
most citedImpact of inter-correlated initial binary parameters on double black hole and neutron star mergers

83 citations · 136 across the 13 of their papers we have counts for

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Showing 2025Show all

7 papers · 1 filter

astro-ph.IM2025

Dynamical binary interactions in the 2040s

Nadejda Blagorodnova, Ondřej Pejcha, Tomek Kamiński +15

Dynamical binary interactions such as common envelope (CE) evolution or stellar mergers are a critical phase in the formation of a wide variety of binary phenomena, ranging from bl…

astro-ph.SR2025

The formation of merging black holes via stable mass transfer in massive binary stars

Xiao-Tian Xu, Norbert Langer, Jakub Klencki +2

The vast majority of massive binary systems in the universe is evidently unsuited to produce merging binary black holes. However, several narrow evolutionary paths of isolated mass…

astro-ph.HE2025

Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System

Aleksandra Olejak, Jakub Klencki, Alejandro Vigna-Gomez +6

The detected Gaia systems hosting compact objects challenge standard models of binary star evolution. In particular, if the observed black hole (BH) systems evolved in isolation, t…

astro-ph.HE2025★ 3 cited

Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium CoreBlack Hole Mergers Following Delayed Dynamical Instability

Jakub Klencki, Brian D. Metzger

Binaries in which a massive donor star undergoes an extended ( kyr) phase of stable mass transfer onto a black hole (BH) accretor offer a promising channel for creating LI…

astro-ph.HE2025★ 12 cited

Orbital Eccentricity and Spin-Orbit Misalignment Are Evidence that Neutron Star-Black Hole Mergers Form through Triple Star Evolution

Jakob Stegmann, Jakub Klencki

There is growing evidence that a substantial fraction of the neutron star-black holes (NSBHs) detected through gravitational waves merge with non-zero eccentricity or large BH spin…

astro-ph.HE2025★ 9 cited

A fundamental limit to how close binary systems can get via stable mass transfer shapes the properties of binary black hole mergers

Jakub Klencki, Philipp Podsiadlowski, Norbert Langer +4

Mass transfer in binary systems is the key process in the formation of various classes of objects, including merging binary black holes (BBHs) and neutron stars. Orbital evolution…

astro-ph.SR2025

Using detailed single star and binary evolution models to probe the large observed luminosity spread of red supergiants in young open star clusters

Chen Wang, Lee Patrick, Abel Schootemeijer +12

Red supergiants (RSGs) represent a late evolutionary stage of massive stars. Recent observations reveal that the observed luminosity range of RSGs in young open clusters is wider t…