activity
20162026
most citedDouble neutron stars: merger rates revisited

204 citations · 978 across the 29 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.SR2023★ 14 cited

On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations

Debasish Dutta, Jakub Klencki

The majority of massive stars are formed in multiple systems and will interact with companions via mass transfer. This interaction typically leads to the primary shedding its envel…

astro-ph.SR2023

Stellar Black Holes and Compact Stellar Remnants

Guglielmo Costa, Martyna Chruślińska, Jakub Klencki +4

The recent observations of gravitational waves (GWs) by the LIGO-Virgo-KAGRA collaboration (LVK) have provided a new opportunity for studying our Universe. By detecting several mer…

astro-ph.SR2023★ 4 cited

Everything that glitters is not gold: V1315 Cas is not a dormant black hole

J. Zak, D. Jones, H. M. J. Boffin +11

The quest for quiet or dormant black holes has been ongoing since several decades. Ellipsoidal variables possibly indicate the existence of a very high-mass invisible companion and…

astro-ph.SR2023★ 30 cited

A partially stripped massive star in a Be binary at low metallicity: A missing link towards Be X-ray binaries and double neutron star mergers

V. Ramachandran, J. Klencki, A. A. C. Sander +4

Standard binary evolutionary models predict a significant population of core helium-burning stars that lost their hydrogen-rich envelope after mass transfer via Roche-lobe overflow…

astro-ph.SR2023★ 61 cited

X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

Jorick S. Vink, A. Mehner, P. A. Crowther +78

Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational-wave events involving spectacular black-hole mergers, indicate that the low…

astro-ph.SR2023★ 14 cited

Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity

D. Pauli, L. M. Oskinova, W. -R. Hamann +16

The origin of the observed population of Wolf-Rayet (WR) stars in low-metallicity (low-Z) galaxies, such as the Small Magellanic Cloud (SMC), is not yet understood. Standard, singl…