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dc.contributorLowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, USA
dc.contributorINAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
dc.contributorArmagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK; Institute of Astronomy and National Astronomical Observatory, Bulgaria Academy of Sciences, 72, Tsarigradsko Chaussee Blvd., BG-1784 Sofia, Bulgaria
dc.contributorUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange UMR7293, Nice, France
dc.contributorArmagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK
dc.contributorUniversité Côte d'Azur, Observatoire de la Côte d'Azur, UMR7293 CNRS Laboratoire Optique, Bv de l'Observatoire, CS 34229, F-06304 Nice, France
dc.contributorInstitute of Astronomy and National Astronomical Observatory, Bulgaria Academy of Sciences, 72, Tsarigradsko Chaussee Blvd., BG-1784 Sofia, Bulgaria
dc.contributorInstitute of Astronomy of Kharkiv National University, Sumska Str. 35, Kharkiv 61022, Ukraine
dc.contributor.authorDevogèle, M.
dc.contributor.authorCellino, A.
dc.contributor.authorBorisov, G.
dc.contributor.authorBendjoya, Ph
dc.contributor.authorRivet, J. -P.
dc.contributor.authorAbe, L.
dc.contributor.authorBagnulo, S.
dc.contributor.authorChristou, A.
dc.contributor.authorVernet, D.
dc.contributor.authorDonchev, Z.
dc.contributor.authorBelskaya, I.
dc.contributor.authorBonev, T.
dc.contributor.authorKrugly, Yu N.
dc.date.accessioned2024-02-01T17:09:51Z
dc.date.available2024-02-01T17:09:51Z
dc.date.issued2018-09-01T00:00:00Z
dc.identifier.doi10.1093/mnras/sty1587
dc.identifier.doi10.48550/arXiv.1806.05277
dc.identifier.other2018arXiv180605277D
dc.identifier.other2018MNRAS.tmp.1645D
dc.identifier.otherastro-ph.EP
dc.identifier.other2018arXiv180605277D
dc.identifier.other10.1093/mnras/sty1587
dc.identifier.otherarXiv:1806.05277
dc.identifier.other2018MNRAS.tmp.1645D
dc.identifier.other10.48550/arXiv.1806.05277
dc.identifier.other2018MNRAS.479.3498D
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1317
dc.description.abstractA multicolour phase-polarization curve of asteroid (3200) Phaethon has been obtained during the 2017 December apparition by merging measurements taken at the observing station of Calern (France) and at the Rozhen observatory (Bulgaria). All the observations were obtained in the positive polarization branch, the phase angle ranging from 36° to 116°. The measured values of linear polarization are among the highest ever observed for a Solar system body. The covered interval of phase angle was not sufficiently extended to derive a firm determination of the P<SUB>max</SUB> parameter, but this appears to occur at a phase angle around 130° and reaches more than 45 per cent of linear polarization. Phaethon is the parent body of the Geminid meteor shower, and the real physical nature of this object (asteroid or comet) has been a long-debated subject. Our polarimetric measurements seem to support the asteroid hypothesis with a phase-polarization curve similar to the asteroid (2) Pallas, but further observations at smaller phase angles are needed to draw definitive conclusions.
dc.publisherMonthly Notices of the Royal Astronomical Society
dc.titleThe phase-polarization curve of asteroid (3200) Phaethon<SUP>†</SUP>
dc.typearticle
dc.source.journalMNRAS
dc.source.journalMNRAS.479
dc.source.volume479
refterms.dateFOA2024-02-01T17:09:51Z
dc.identifier.bibcode2018MNRAS.479.3498D


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