activity
20062023
most citedPossible planet-forming regions on submillimetre images

189 citations · 693 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.EP2023★ 5 cited

Mitigating potentially hazardous asteroid impacts revisited

Zs. Regaly, V. Frohlich, P. Berczik

Context: Potentially hazardous asteroids (PHA) in Earth-crossing orbits pose a constant threat to life on Earth. Several mitigation methods have been proposed, and the most feasibl…

astro-ph.EP2023★ 3 cited

Planetary nurseries: vortices formed at smooth viscosity transition

Zs. Regaly, K. Kadam, D. Tarczay-Nehez

Excitation of Rossby wave instability and development of a large-scale vortex at the outer dead zone edge of protoplanetary discs is one of the leading theories that explains horse…

astro-ph.SR2022★ 6 cited

Lost in space: companions' fatal dance around massive dying stars

Zsolt Regaly, Viktoria Frohlich, Jozsef Vinko

Discoveries of planet- and stellar remnant-hosting pulsars challenge our understanding as the violent supernova explosion that forms the pulsar presumably destabilizes the system.…

astro-ph.SR2022★ 1 cited

A gap at 1 au in the disk of DI Cha A revealed by infrared interferometry

Tímea Juhász, Péter Ábrahám, Attila Moór +6

DI Cha A is K0-type pre-main sequence star, the brightest component of a quadruple stellar system. Here we report on a detailed study of this star based on archival VLTI/MIDI and V…

astro-ph.EP2021★ 10 cited

Self-Sustaining Vortices in Protoplanetary Disks: Setting the Stage for Planetary System Formation

Zsolt Regaly, Kundan Kadam, Cornelis P. Dullemond

The core accretion scenario of planet formation assumes that planetesimals and planetary embryos are formed during the primordial, gaseous phases of the protoplanetary disk. Howeve…

astro-ph.EP2021★ 5 cited

Increased isolation mass for pebble accreting planetary cores in pressure maxima of protoplanetary discs

Zsolt Sándor, Zsolt Regály

The growth of a pebble accreting planetary core is stopped when reaching its \textit{isolation mass} that is due to a pressure maximum emerging at the outer edge of the gap opened…