activity
20092017
most citedA characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA

513 citations · 1.2k across the 19 of their papers we have counts for

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Showing astro-ph.EPShow all

6 papers · 1 filter

astro-ph.EP2017★ 34 cited

Capture of exocomets and the erosion of the Oort cloud due to stellar encounters in the Galaxy

Joris Hanse, Lucie Jilkova, Simon F. Portegies Zwart +1

The Oort cloud (OC) probably formed more than 4Gyr ago and has been moving with the Sun in the Galaxy since, exposed to external influences, most prominently to the Galactic ti…

astro-ph.EP2016★ 33 cited

The rate of stellar encounters along a migrating orbit of the Sun

C. A. Martínez-Barbosa, L. Jílková, S. Portegies Zwart +1

The frequency of Galactic stellar encounters the Solar system experienced depends on the local density and velocity dispersion along the orbit of the Sun in the Milky Way galaxy. W…

astro-ph.EP2016★ 43 cited

Mass transfer between debris discs during close stellar encounters

Lucie Jilkova, Adrian S. Hamers, Michael Hammer +1

We study mass transfers between debris discs during stellar encounters. We carried out numerical simulations of close flybys of two stars, one of which has a disc of planetesimals…

astro-ph.EP2015★ 74 cited

How Sedna and family were captured in a close encounter with a solar sibling

Lucie Jilkova, Simon Portegies Zwart, Tjibaria Pijloo +1

The discovery of 2012VP113 initiated the debate on the origin of the Sedna family of planetesimals in orbit around the Sun. Sednitos roam the outer regions of the Solar System betw…

astro-ph.EP2015★ 60 cited

The fragility of planetary systems

Simon Portegies Zwart, Lucie Jilkova

We specify the range to which perturbations penetrate a planetesimal system. Such perturbations can originate from massive planets or from encounters with other stars. The latter c…

astro-ph.EP2015★ 24 cited

A debris disk under the influence of a wide planetary mass companion: The system of HD106906

Lucie Jilkova, Simon Portegies Zwart

The 13 Myr old star HD106906 is orbited by a debris disk of at least 0.067 M_Moon with an inner and outer radius of 20 AU and 120 AU, respectively, and by a planet at a distance of…