Počet záznamů: 1
The young Datura asteroid family Spins, shapes, and population estimate
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SYSNO ASEP 0485038 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název The young Datura asteroid family Spins, shapes, and population estimate Tvůrce(i) Vokrouhlický, D. (CZ)
Pravec, Petr (ASU-R) RID, ORCID
Ďurech, J. (CZ)
Bolin, B. (FR)
Jedicke, R. (US)
Kušnirák, Peter (ASU-R)
Galád, Adrián (ASU-R) RID
Hornoch, Kamil (ASU-R) ORCID
Kryszczynska, A. (PL)
Colas, F. (FR)
Moskovitz, N. (US)
Thirouin, A. (ES)
Nesvorný, D. (US)Zdroj.dok. Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 598, February (2017), A91/1-A91/19Poč.str. 19 s. Forma vydání Online - E Jazyk dok. eng - angličtina Země vyd. FR - Francie Klíč. slova celestial mechanics ; minor planets ; asteroids Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP GAP209/12/0229 GA ČR - Grantová agentura ČR Institucionální podpora ASU-R - RVO:67985815 UT WOS 000394465000090 EID SCOPUS 85012093994 DOI 10.1051/0004-6361/201629670 Anotace We study the most suitable known asteroid family with an age of less than 1 Myr, the Datura family. We aim (i) to obtain information about rotation state and shape of the largest members in the family and (ii) to constrain its debiased population down to couple of hundreds of meters in size. We have analyzed the up-to-date catalog of orbital elements of main belt asteroids. We evaluated the detection efficiency of Catalina Sky Survey (CSS) in regard to detections of members in the Datura family, and we have used our photometric observations and lightcurve inversion methods to determine the rotation states and shapes of the largest members of the family. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2018
Počet záznamů: 1