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Amaro, P.Cuadra, Jorge.[The butterfly effect in the extreme-mass ratio inspiral problem]The butterfly effect in the extreme-mass ratio inspiral problem

Baruteau, C.Cuadra, Jorge.[BINARIES MIGRATING IN A GASEOUS DISK: WHERE ARE THE GALACTIC CENTER BINARIES?]BINARIES MIGRATING IN A GASEOUS DISK: WHERE ARE THE GALACTIC CENTER BINARIES?

Amaro Seoane, P.Cuadra, Jorge.[TIDAL DISRUPTIONS IN CIRCUMBINARY DISKS. I. STAR FORMATION, DYNAMICS, AND BINARY EVOLUTION]TIDAL DISRUPTIONS IN CIRCUMBINARY DISKS. I. STAR FORMATION, DYNAMICS, AND BINARY EVOLUTION

Casassus, S.Jordán Colzani, Andres Cristóbal.Cuadra, Jorge.[The dynamically disrupted gap in HD 142527]The dynamically disrupted gap in HD 142527

Nayakshin, S.Cuadra, Jorge.[Simulations of star formation in a gaseous disc around Sgr A*- a failed Active Galactic Nucleus]Simulations of star formation in a gaseous disc around Sgr A*- a failed Active Galactic Nucleus

Alexander, R.D.Cuadra, Jorge.[Self-Gravitating Fragmentation of Eccentric Accretion Disks]Self-Gravitating Fragmentation of Eccentric Accretion Disks

Alexander, R.D.Cuadra, Jorge.[Binary formation and mass function variations in fragmenting discs with short cooling times]Binary formation and mass function variations in fragmenting discs with short cooling times

Paumard, T.Cuadra, Jorge.[The two young star disks in the central parsec of the Galaxy: properties, dynamics, and formation]The two young star disks in the central parsec of the Galaxy: properties, dynamics, and formation

The source G2 has already completed its pericentre passage around Sgr A*, the supermassive black hole in the centre of our Galaxy. Although it has been monitored for 15 yr, its astrophysical nature and origin still remain unknown. In this work, we aim to test the hypothesis of G2 being the result...


Calderón Espinoza, DiegoCuadra, Jorge.Schartmann, MarcBurkert, AndreasPlewa, P.Eisenhauer, F.Habibi, M.[The Galactic Centre source G2 was unlikely born in any of the known massive binaries]The Galactic Centre source G2 was unlikely born in any of the known massive binaries

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