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19932026
most citedCometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites

524 citations · 4k across the 63 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 60 cited

On a Scattered-Disk Origin for the 2003 El61 Collisional Family - an Example of the Importance of Collisions on the Dynamics of Small Bodies

Harold F. Levison, Morbidelli Alessandro, David Vokrouhlicky +1

The recent discovery of the 2003EL61 collisional family in the Kuiper belt (Brown et al., 2007) is surprising because the formation of such a family is a highly improbable event in…

astro-ph2007★ 13 cited

LSST: Comprehensive NEO Detection, Characterization, and Orbits

Z. Ivezic, J. A. Tyson, M. Juric +6

(Abridged) The Large Synoptic Survey Telescope (LSST) is currently by far the most ambitious proposed ground-based optical survey. Solar System mapping is one of the four key scien…

astro-ph2003★ 391 cited

The IAU 2000 resolutions for astrometry, celestial mechanics and metrology in the relativistic framework: explanatory supplement

M. Soffel, S. A. Klioner, G. Petit +17

This paper discusses the IAU Resolutions B1.3, B1.4, B1.5 and B1.9 (2000) that were adopted during the 24th General Assembly in Manchester, 2000 and provides details and explanatio…

astro-ph1998★ 35 cited

Stellar dynamics in a galactic centre surrounded by a massive accretion disc. I. Newtonian description

D. Vokrouhlicky, V. Karas

The long-term evolution of stellar orbits bound to a massive centre is studied in order to understand the cores of star clusters in central regions of galaxies. Stellar trajectorie…

astro-ph1994★ 7 cited

Emission Line Profiles from Self-Gravitating Thin Disks

V. Karas, A. Lanza, D. Vokrouhlicky

We have constructed general relativistic models of a stationary, axially symmnetric, Keplerian thin disk around a rotating black hole. We computed profiles of a spectral line, emit…

astro-ph1993

Motion of a Solar Mass Compact Object Around a Massive Rotating Black Hole

V. Karas, D. Vokrouhlicky

This preprint is based on two articles accepted by MNRAS and ApJ. Our aim is to study the evolution of the orbit of a star under the influence of interactions with an accretion dis…