activity
20102024
most citedFormation of asteroid pairs by rotational fission

214 citations · 294 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP202410 cited

Size, albedo and rotational period of the Hayabusa2# target (98943) 2001 CC21

S. Fornasier, E. Dotto, P. Panuzzo +8

This study aims to determine the size, albedo and rotational period of (98943) 2001 CC21, target of the Hayabusa2 extended mission, using thermal data from the Spitzer Space telesc…

astro-ph.EP20231 cited

Photometry of the Didymos system across the DART impact apparition

Nicholas Moskovitz, Cristina Thomas, Petr Pravec +78

On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the satellite of binary near-Earth asteroid (65803) Didymos. This demonstrated the…

astro-ph.EP202323 cited

A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS measured from stellar occultations

F. L. Rommel, F. Braga-Ribas, J. L. Ortiz +201

This work aims at constraining the size, shape, and geometric albedo of the dwarf planet candidate 2002 MS4 through the analysis of nine stellar occultation events. Using multichor…

astro-ph.EP2023

Physical modelling of near-Earth asteroid (23187) 2000 PN9 with ground-based optical and radar observations

L. Dover, S. C. Lowry, A. Rożek +19

We present a physical model and spin-state analysis of the potentially hazardous asteroid (23187) 2000 PN9. As part of a long-term campaign to make direct detections of the YORP ef…

astro-ph.HE201646 cited

Multicolour modelling of SN 2013dx associated with GRB 130702A

A. A. Volnova, M. V. Pruzhinskaya, A. S. Pozanenko +13

We present optical observations of SN 2013dx, related to the Fermi burst GRB 130702A occurred at a redshift z = 0.145. It is the second-best sampled GRB-SN after SN~1998bw: the obs…

astro-ph.EP2010214 cited

Formation of asteroid pairs by rotational fission

P. Pravec, D. Vokrouhlicky, D. Polishook +23

Asteroid pairs sharing similar heliocentric orbits were found recently. Backward integrations of their orbits indicated that they separated gently with low relative velocities, but…