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researcher

D. Vokrouhlický

63 papers hereh-index 6714.8k citations359 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author37
  • last author17

Across the 58 of 63 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP51
  • astro-ph6
  • astro-ph.SR4
  • astro-ph.GA1
  • gr-qc1
same name
  • D. Vokrouhlický — 19 papers, h 14
  • D. Vokrouhlický — 12 papers, h 7
  • D. Vokrouhlický — 7 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19932026
most citedCometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites

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

collaborators
Showing 2020Show all

4 papers · 1 filter

astro-ph.EP2020

Clarissa Family Age from the Yarkovsky Effect Chronology

Vanessa C. Lowry, David Vokrouhlicky, David Nesvorny +1

The Clarissa family is a small collisional family composed of primitive C-type asteroids. It is located in a dynamically stable zone of the inner asteroid belt. In this work we det…

astro-ph.EP2020★ 50 cited

OSSOS XX: The Meaning of Kuiper Belt Colors

David Nesvorny, David Vokrouhlicky, Mike Alexandersen +9

Observations show that 100-km-class Kuiper belt objects (KBOs) can be divided in (at least) two color groups, hereafter red (R, g-i<1.2) and very red (VR, g-i>1.2), reflecting a di…

astro-ph.EP2020★ 8 cited

Analytical solution of the Colombo top problem

J. Haponiak, S. Breiter, D. Vokrouhlicky

The Colombo top is a basic model in the rotation dynamics of a celestial body moving on a precessing orbit and perturbed by a gravitational torque. The paper presents a detailed st…

astro-ph.EP2020★ 14 cited

Very Slow Rotators from Tidally Synchronized Binaries

D. Nesvorny, D. Vokrouhlicky, W. F. Bottke +2

A recent examination of K2 lightcurves indicates that ~15% of Jupiter Trojans have very slow rotation (spin periods Ps>100 h). Here we consider the possibility that these bodies fo…

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