Title
Do Slivan states exist in the Flora family?: I. Photometric survey of the Flora region
Date Issued
15 October 2012
Access level
open access
Resource Type
journal article
Author(s)
Kryszczyńska A.
Polińska M.
Hirsch R.
Ivanova V.
Apostolovska G.
Bilkina B.
Velichko F.P.
Kwiatkowski T.
Kankiewicz P.
Vachier F.
Umlenski V.
Michałowski T.
Marciniak A.
Maury A.
Kamiński K.
Fagas M.
Dimitrov W.
Borczyk W.
Sobkowiak K.
Lecacheux J.
Behrend R.
Klotz A.
Bernasconi L.
Crippa R.
Manzini F.
Poncy R.
Antonini P.
Oszkiewicz D.
Santana-Ros T.
Observatoire de Paris
Abstract
Context. Recent studies have uncovered evidence that the statistical properties of asteroids' physical parameters are a fundamental source of information on the physics of their collisions and evolution. The analysis of the spin rates and spin vector distributions helps us to understand the role of various known and new effects. The alignment of spin vectors and the correlation of spin rates are for the first time observed for ten members of the Koronis family. These unexpected non-random orientations of the spin axes and correlations of the spin rates, now known as Slivan states are interpreted in terms of a YORP effect and spin-orbit resonances. Aims. To study non-gravitational-effects, there appears to be a need for new observational campaigns devoted to determining the physical parameters of the asteroid families. Methods. We analysed the photometric observations of the asteroids, which are the most efficient method of studying asteroid physical parameters. Results. We report the results of a ten-year long observational survey of the light variations of objects in the Flora region. We present 544 individual lightcurves of 55 objects obtained at various observing geometries. These lightcurves yield new or refined synodic periods for 32 asteroids and confirm period determinations for 23 objects in our sample. To improve the statistics of the Flora family objects, we add to our dataset 91 objects with reliably determined periods. The distribution of rotation rates for the Flora family is non-Maxwellian at a confidence level of 94% and different from those of the Koronis and the Hungaria families. It seems to be consistent with the long-term influence of the YORP effect, although it is also indicative of a younger age for the Flora family compared to both the Koronis and the Hungaria families. Conclusions. Our new data is a foundation for the spin vector and shape determinations that will be the objectives of the second paper of the series. We search for spin vector and spin periods correlations in order to determine whether Slivan states exist in the Flora family. ©2012 ESO.
Volume
546
Language
English
OCDE Knowledge area
Astronomía
Subjects
Scopus EID
2-s2.0-84867257240
Source
Astronomy and Astrophysics
ISSN of the container
14320746
Sponsor(s)
A.K. and M.P. thank Iwona Wytrzyszczak for her help with the Kolmogorov-Smirnov test. A.K. was supported by the Polish Grant N N203 382136, M.P. was supported by the Polish Grant N N203 387937, G.A. gratefully acknowledge observing grant support from the Institute of Astronomy and Rozhen National Astronomical Observatory, Bulgarian Academy of Sciences. V.A. was partially supported by a contract DO 02-85 between the Institute of Astronomy from Bulgarian Academy of Science and Bulgarian Ministry of Education, Youth, and Science. Observations of 4150 Starr and 1667 Pels were made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. The work of TSR was carried out through the Gaia Research for European Astronomy Training (GREAT-ITN) network. He received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 264895. This work is partially based on observations made at the South African Astronomical Observatory (SAAO). The reduction of most of the CCD data was performed with the CCLR STARLINK package.
Sources of information:
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