Shape and spin determination of Barbarian asteroids

DEVOGELE, M.; TANGA, P.; BENDJOYA, P.; RIVET, J.; SURDEJ, J.; HANUS, J.; ABE, L.; ANTONINI, P.; ARTOLA, R.; AUDEJEAN, M.; Behrend, R.; BERSKI, F.; BOSCH, J.; BRONIKOWSKA, M.; CARBOGNANI, A.; Char, F.; Kim, M.; Choi, Y.; COLAZO, C.; COLOMA, J.; COWARD, D.; DURKEE, R.; ERECE, O.; FORNE, E.; Hickson, P.; HIRSCH, R.; HORBOWICZ, J.; KAMINSKI, K.; KANKIEWICZ, P.; KAPLAN, MURAT; KWIATKOWSKI, T.; KONSTANCIAK, I.; KRUSZEWKI, A.; KUDAK, V.; MANZINI, F.; Moon, H.; MARCINIAK, A.; MURAWIECKA, M.; Nadolny, J.; OGLOZA, W.; ORTIZ, J.; OSZKIEWICZ, D.; PALLARES, H.; Peixinho, N.; PONCY, R.; REYES, F.; DE LOS REYES, J.; SANTANA-ROS, T.; SOBKOWIAK, K.; PASTOR, S.; PILCHER, F.; QUINONES, M.; TRELA, P.; VERNET, D.

doi:10.1051/0004-6361/201630104

Shape and spin determination of Barbarian asteroids

Atıf İçin Kopyala

DEVOGELE M., TANGA P., BENDJOYA P., RIVET J. P., SURDEJ J., HANUS J., ...Daha Fazla

ASTRONOMY & ASTROPHYSICS, cilt.607, 2017 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 607
Basım Tarihi: 2017
Doi Numarası: 10.1051/0004-6361/201630104
Dergi Adı: ASTRONOMY & ASTROPHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Anahtar Kelimeler: techniques: photometric, minor planets, asteroids: general, methods: observational, MAIN-BELT ASTEROIDS, LIGHTCURVE INVERSION, PHOTOELECTRIC PHOTOMETRY, POLARIMETRIC BEHAVIOR, OPTIMIZATION METHODS, NONCONVEX, PERIODS, MODELS
Akdeniz Üniversitesi Adresli: Evet

Özet

Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barbara, the first on which such properties were identified. As has been suggested, large scale topographic features could play a role in the polarimetric response, if the shapes of Barbarians are particularly irregular and present a variety of scattering/incidence angles. This idea is supported by the shape of (234) Barbara, that appears to be deeply excavated by wide concave areas revealed by photometry and stellar occultations.