activity
20202026
most citedPolluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries

115 citations · 174 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Continuous mass ablation of planets engulfed in stellar envelopes

Mike Y. M. Lau, Robert Andrassy, Giovanni Leidi +4

Most stars host short-period planets that are expected to be engulfed during post-main-sequence expansion. The dissolution of engulfed planets has been proposed as a possible mecha…

astro-ph.SR2026

Localized O production in white dwarf mergers

Alexander Holas, Veronica Agaeva, Friedrich K. Roepke +5

The merger of a He white dwarf (WD) and a CO WD is the favored formation channel for R Coronae Borealis (RCB) stars. These stars exhibit ratio…

gr-qc2024★ 39 cited

The Lunar Gravitational-wave Antenna: Mission Studies and Science Case

Parameswaran Ajith, Pau Amaro Seoane, Manuel Arca Sedda +83

The Lunar Gravitational-wave Antenna (LGWA) is a proposed array of next-generation inertial sensors to monitor the response of the Moon to gravitational waves (GWs). Given the size…

astro-ph.SR2024★ 2 cited

Thermonuclear explosions as Type II supernovae

Alexandra Kozyreva, Javier Moran-Fraile, Alexander Holas +5

We consider a binary stellar system, in which a low-mass, of 0.6 Msun, carbon-oxygen white dwarf (WD) mergers with a degenerate helium core of 0.4 Msun of a red giant. We analyse t…

astro-ph.SR2023★ 1 cited

Faint calcium-rich transient from the double-detonation of a carbon-oxygen white dwarf star

J. Moran-Fraile, A. Holas, F. K. Roepke +2

We have computed a three-dimensional hydrodynamic simulation of the merger between a massive () helium white dwarf (He WD) and a low-mass () carbon-oxyg…

astro-ph.HE2023★ 17 cited

Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger

J. Moran-Fraile, F. K. Roepke, R. Pakmor +4

The merger of a white dwarf (WD) and a neutron star (NS) is a relatively common event that will produce an observable electromagnetic signal. Furthermore, the compactness of these…