2007A&A...465..331D


Query : 2007A&A...465..331D

2007A&A...465..331D - Astronomy and Astrophysics, volume 465, 331-337 (2007/4-1)

Physical models of ten asteroids from an observers' collaboration network.

DURECH J., KAASALAINEN M., MARCINIAK A., ALLEN W.H., BEHREND R., BEMBRICK C., BENNETT T., BERNASCONI L., BERTHIER J., BOLT G., BOROUMAND S., CRESPO DA SILVA L., CRIPPA R., CROW M., DURKEE R., DYMOCK R., FAGAS M., FAUERBACH M., FAUVAUD S., FREY M., GONCALVES R., HIRSCH R., JARDINE D., KAMINSKI K., KOFF R., KWIATKOWSKI T., LOPEZ A., MANZINI F., MICHALOWSKI T., PACHECO R., PAN M., PILCHER F., PONCY R., PRAY D., PYCH W., ROY R., SANTACANA G., SLIVAN S., SPOSETTI S., STEPHENS R., WARNER B. and WOLF M.

Abstract (from CDS):

We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys. The lightcurve inversion method was used to derive spin states and shape models of the asteroids. We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred.

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Journal keyword(s): minor planets, asteroids

VizieR on-line data: <Available at CDS (J/A+A/465/331): objects.dat lc/*>

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2022.05.28-08:38:01

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