The phase-polarization curve of asteroid (3200) Phaethon<SUP>†</SUP>
| dc.contributor | Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, USA | |
| dc.contributor | INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy | |
| dc.contributor | Armagh 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.contributor | Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange UMR7293, Nice, France | |
| dc.contributor | Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK | |
| dc.contributor | Université Côte d'Azur, Observatoire de la Côte d'Azur, UMR7293 CNRS Laboratoire Optique, Bv de l'Observatoire, CS 34229, F-06304 Nice, France | |
| dc.contributor | Institute of Astronomy and National Astronomical Observatory, Bulgaria Academy of Sciences, 72, Tsarigradsko Chaussee Blvd., BG-1784 Sofia, Bulgaria | |
| dc.contributor | Institute of Astronomy of Kharkiv National University, Sumska Str. 35, Kharkiv 61022, Ukraine | |
| dc.contributor.author | Devogèle, M. | |
| dc.contributor.author | Cellino, A. | |
| dc.contributor.author | Borisov, G. | |
| dc.contributor.author | Bendjoya, Ph | |
| dc.contributor.author | Rivet, J. -P. | |
| dc.contributor.author | Abe, L. | |
| dc.contributor.author | Bagnulo, S. | |
| dc.contributor.author | Christou, A. | |
| dc.contributor.author | Vernet, D. | |
| dc.contributor.author | Donchev, Z. | |
| dc.contributor.author | Belskaya, I. | |
| dc.contributor.author | Bonev, T. | |
| dc.contributor.author | Krugly, Yu N. | |
| dc.date.accessioned | 2024-02-01T17:09:51Z | |
| dc.date.available | 2024-02-01T17:09:51Z | |
| dc.date.issued | 2018-09-01T00:00:00Z | |
| dc.identifier.doi | 10.1093/mnras/sty1587 | |
| dc.identifier.doi | 10.48550/arXiv.1806.05277 | |
| dc.identifier.other | 2018arXiv180605277D | |
| dc.identifier.other | 2018MNRAS.tmp.1645D | |
| dc.identifier.other | astro-ph.EP | |
| dc.identifier.other | 2018arXiv180605277D | |
| dc.identifier.other | 10.1093/mnras/sty1587 | |
| dc.identifier.other | arXiv:1806.05277 | |
| dc.identifier.other | 2018MNRAS.tmp.1645D | |
| dc.identifier.other | 10.48550/arXiv.1806.05277 | |
| dc.identifier.other | 2018MNRAS.479.3498D | |
| dc.identifier.other | - | |
| dc.identifier.uri | http://hdl.handle.net/20.500.14302/1317 | |
| dc.description.abstract | A 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.publisher | Monthly Notices of the Royal Astronomical Society | |
| dc.title | The phase-polarization curve of asteroid (3200) Phaethon<SUP>†</SUP> | |
| dc.type | article | |
| dc.source.journal | MNRAS | |
| dc.source.journal | MNRAS.479 | |
| dc.source.volume | 479 | |
| refterms.dateFOA | 2024-02-01T17:09:51Z | |
| dc.identifier.bibcode | 2018MNRAS.479.3498D |

