activity
20092026
most citedAnalysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger - search for the YORP effect

44 citations · 249 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2026

The Inbound Gas and Dust Evolution of Interstellar Comet 3I/ATLAS from Optical Spectroscopy and Multi-band Photometry

Toni Santana-Ros, Alexey Sergeyev, Oleksandra Ivanova +9

Interstellar objects (ISOs) provide direct constraints on the composition and evolution of extrasolar planetary systems. As the third confirmed ISO, comet 3I/ATLAS offers a rare op…

astro-ph.EP2024★ 10 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.EP2023★ 1 cited

Secular change in the spin states of asteroids due to radiation and gravitation torques. New detections and updates of the YORP effect

J. Ďurech, D. Vokrouhlický, P. Pravec +21

The rotation state of small asteroids is affected in the long term by perturbing torques of gravitational and radiative origin (the YORP effect). Direct observational evidence of t…

astro-ph.EP2023★ 23 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.EP2022★ 18 cited

Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation

P. Santos-Sanz, J. L. Ortiz, B. Sicardy +85

Within our international program to obtain accurate physical properties of trans-Neptunian objects (TNOs) we predicted a stellar occultation by the TNO (38628) Huya of the star Gai…

astro-ph.EP2022★ 11 cited

Polarimetry of M-type asteroids in the context of their surface composition

I. Belskaya, A. Berdyugin, Yu. Krugly +9

Aims. We aim to investigate how polarimetric observations can improve our understanding of the nature and diversity of M/X-type asteroids. Methods. Polarimetric observations of the…

astro-ph.EP2022

Observations of asteroid magnitude-phase relations at the Kharadze Abastumani Astrophysical Observatory

V. G. Shevchenko1, R. Ya. Inasaridze, Yu. N. Krugly +6

In frame of an implementation of the cooperative program studying of asteroids between the Kharadze Abastumani Astrophysical Observatory and the Astronomical Institute of V.N. Kara…

astro-ph.EP2021★ 18 cited

Rotation acceleration of asteroids (10115) 1992 SK, (1685) Toro, and (1620) Geographos due to the YORP effect

J. Durech, D. Vokrouhlicky, P. Pravec +28

The rotation state of small asteroids is affected by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, which is a net torque caused by solar radiation directly reflected and…

astro-ph.EP2021★ 9 cited

Photometry of selected outer main belt asteroids

V. Shevchenko, O. Mikhalchenko, I. Belskaya +17

We present new photometric observations for twelve asteroids ((122) Gerda, (152) Atala, (260) Huberta, (665) Sabine, (692) Hippodamia, (723) Hammonia, (745) Mauritia, (768) Struvea…

astro-ph.EP2021★ 6 cited

Small solar system objects on highly inclined orbits: Surface colours and lifetimes

T. Hromakina, I. Belskaya, Yu. Krugly +9

Less than one percent of the discovered small solar system objects have highly inclined orbits (), and revolve around the Sun on near-polar or retrograde orbits. The…

astro-ph.EP2018★ 29 cited

Rotational variation of the linear polarisation of the asteroid (3200) Phaethon as evidence for inhomogeneity in its surface properties

G. Borisov, M. Devogèle, A. Cellino +23

Asteroid (3200) Phaethon is a Near-Earth Apollo asteroid with an unusual orbit that brings it closer to the Sun than any other known asteroid. Its last close approach to the Earth…

astro-ph.EP2018★ 40 cited

The phase-polarization curve of asteroid (3200) Phaethon

M. Devogèle, A. Cellino, G. Borisov +10

A multi-colour phase-polarization curve of asteroid (3200)~Phaethon has been obtained during the December 2017 apparition by merging measurements taken at the observing station of…

astro-ph.EP2015★ 14 cited

The astrometric Gaia-FUN-SSO observation campaign of 99 942 Apophis

W. Thuillot, D. Bancelin, A. Ivantsov +71

Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gaia-FUN-SSO) play a key role in ensuring that moving objects first detected by ESA's Gai…

astro-ph.EP2012★ 44 cited

Analysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger - search for the YORP effect

J. Durech, D. Vokrouhlicky, A. R. Baransky +28

The spin state of small asteroids can change on a long timescale by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, the net torque that arises from anisotropically scatter…

astro-ph.HE2009★ 26 cited

Multi-wavelength observations of afterglow of GRB 080319B and the modeling constraints

S. B. Pandey, A. J. Castro-Tirado, M. Jelínek +24

We present observations of the afterglow of GRB 080319B at optical, mm and radio frequencies from a few hours to 67 days after the burst. Present observations along with other publ…