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相关论文: Fraction of Contact Binary Trojan Asteroids

200 篇论文

We have observed well-sampled phase curves for nine Trojan asteroids in B-, V-, and I-bands. These were constructed from 778 magnitudes taken with the 1.3-m telescope on Cerro Tololo as operated by a service observer for the SMARTS…

地球与行星天体物理 · 物理学 2015-05-14 Martha W. Schaefer , Bradley E. Schaefer , David L. Rabinowitz , Suzanne W. Tourtellotte

We fit 54,296 sparsely-sampled asteroid lightcurves in the Palomar Transient Factory to a combined rotation plus phase-function model. Each lightcurve consists of 20+ observations acquired in a single opposition. Using 805 asteroids in our…

We present mid-infrared (8-33 micron) observations of the binary L5-Trojan system (617) Patroclus-Menoetius before, during, and after two shadowing events, using the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope.F or the…

Photometric observations and analysis of twelve previously poorly studied contact binary systems is presented. All show total eclipses and have extremely low mass ratios ranging from 0.072 to 0.15. Also, all show characteristics of orbital…

We present the first results obtained from an extensive study of eclipsing binary (EB) system candidates recently detected in the VISTA Variables in the V\'ia L\'actea (VVV) near-infrated (NIR) Survey. We analyze the VVV tile d040 in the…

太阳与恒星天体物理 · 物理学 2020-12-16 L. V. Gramajo , T. Palma , D. Minniti , R. K. Saito , J. J. Clariá , R. Kammers , F. Surot

Binary systems comprise approximately 15 per cent of the near-Earth asteroid population, yet thermal-infrared data are often interpreted for these bodies as if they are single objects. Thermal-IR light curves of binary asteroids (3905)…

地球与行星天体物理 · 物理学 2024-09-20 Samuel L. Jackson , Benjamin Rozitis

We present the results of a high-resolution imaging survey for brown dwarf binaries in the Pleiades open cluster. The observations were carried out with the Advance Camera for Surveys onboard the Hubble Space Telescope. Our sample consists…

天体物理学 · 物理学 2009-11-13 H. Bouy , E. Moraux , J. Bouvier , W. Brandner , E. L. Martin , F. Allard , I. Baraffe , M. Fernandez

We present the preliminary analysis of over 1739 known and 349 candidate Jovian Trojans observed by the NEOWISE component of the Wide-field Infrared Survey Explorer (WISE). With this survey the available diameters, albedos and beaming…

We present an analysis of survey observations of the trailing L5 Jupiter Trojan swarm using the wide-field Hyper Suprime-Cam CCD camera on the 8.2 m Subaru Telescope. We detected 189 L5 Trojans from our survey that covered about 15 deg^2 of…

地球与行星天体物理 · 物理学 2022-04-20 Kotomi Uehata , Tsuyoshi Terai , Keiji Ohtsuki , Fumi Yoshida

We report on 176 close (<2") stellar companions detected with high-resolution imaging near 170 hosts of Kepler Objects of Interest. These Kepler targets were prioritized for imaging follow-up based on the presence of small planets, so most…

Asteroid pairs had a single progenitor that split due to rotational-fission of a weak, rubble-pile structured body. By constructing shape models of asteroid pairs from multiple-apparition observations and using a lightcurve inversion…

地球与行星天体物理 · 物理学 2019-11-06 David Polishook , Oded Aharonson

Observational searches for asteroids orbiting near Earth's triangular Lagrange points face unique obstacles. A population of such asteroids would occupy a large projected area on the sky (possibly hundreds of square degrees) and is not…

天体物理学 · 物理学 2009-10-31 Paul Wiegert , Kimmo Innanen , Seppo Mikkola

Recent observations (Burnes2002,Veillet2002,Margot2002a) have revealed an unexpectedly high binary fraction among the Trans-Neptunian Objects (TNOs) that populate the Kuiper Belt. The TNO binaries are strikingly different from asteroid…

天体物理学 · 物理学 2007-05-23 Yoko Funato , Junichiro Makino , Piet Hut , Eiichiro Kokubo , Daisuke Kinoshita

With the aim of investigating the binary population of the 700 Myr old Praesepe cluster, we have observed 149 G and K-type cluster members using adaptive optics. We detected 26 binary systems with an angular separation ranging from less…

天体物理学 · 物理学 2009-11-06 J. Bouvier , G. Duchene , J. -C. Mermilliod , T. Simon

We investigated the probability that an inelastic collision of planetesimals within the Hill sphere of the Jovian planets could explain the presence and orbits of observed irregular satellites. Capture of satellites via this mechanism is…

地球与行星天体物理 · 物理学 2015-05-27 F. Elliott Koch , Bradley M. S. Hansen

We present the results of a high-resolution imaging survey of 22 brown dwarfs and very low mass stars in the nearby (~145 pc) young (~1-2 Myr) low-density star-forming region Taurus-Auriga. We obtained images with the Advanced Camera for…

天体物理学 · 物理学 2008-11-26 A. L. Kraus , R. J. White , L. A. Hillenbrand

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs are poorly understood. The multiplicity properties and minimum mass of the brown-dwarf mass function provide critical…

太阳与恒星天体物理 · 物理学 2015-06-15 J. -Y. Choi , C. Han , A. Udalski , T. Sumi , B. S. Gaudi , A. Gould , D. P. Bennett , M. Dominik , J. -P. Beaulieu , Y. Tsapras , V. Bozza , F. Abe , I. A. Bond , C. S. Botzler , P. Chote , M. Freeman , A. Fukui , K. Furusawa , Y. Itow , C. H. Ling , K. Masuda , Y. Matsubara , N. Miyake , Y. Muraki , K. Ohnishi , N. J. Rattenbury , To. Saito , D. J. Sullivan , K. Suzuki , W. L. Sweatman , D. Suzuki , S. Takino , P. J. Tristram , K. Wada , P. C. M. Yock , M. K. Szymański , M. Kubiak , G. Pietrzyński , I. Soszyński , J. Skowron , S. Kozłowski , R. Poleski , K. Ulaczyk , Ł. Wyrzykowski , P. Pietrukowicz , L. A. Almeida , D. L. DePoy , Subo Dong , E. Gorbikov , F. Jablonski , C. B. Henderson , K. -H. Hwang , J. Janczak , Y. -K. Jung , S. Kaspi , C. -U. Lee , U. Malamud , D. Maoz , D. McGregor , J. A. Munoz , B. -G. Park , H. Park , R. W. Pogge , Y. Shvartzvald , I. -G. Shin , J. C. Yee , K. A. Alsubai , P. Browne , M. J. Burgdorf , S. Calchi Novati , P. Dodds , X. -S. Fang , F. Finet , M. Glitrup , F. Grundahl , S. -H. Gu , S. Hardis , K. Harpsøe , T. C. Hinse , A. Hornstrup , M. Hundertmark , J. Jessen-Hansen , U. G. Jørgensen , N. Kains , E. Kerins , C. Liebig , M. N. Lund , M. Lundkvist , G. Maier , L. Mancini , M. Mathiasen , M. T. Penny , S. Rahvar , D. Ricci , G. Scarpetta , J. Skottfelt , C. Snodgrass , J. Southworth , J. Surdej , J. Tregloan-Reed , J. Wambsganss , O. Wertz , F. Zimmer , M. D. Albrow , E. Bachelet , V. Batista , S. Brillant , A. Cassan , A. A. Cole , C. Coutures , S. Dieters , D. Dominis Prester , J. Donatowicz , P. Fouqué , J. Greenhill , D. Kubas , J. -B. Marquette , J. W. Menzies , K. C. Sahu , M. Zub , D. M. Bramich , K. Horne , I. A. Steele , R. A. Street

We present the results of a visible spectroscopic and photometric survey of Jupiter Trojans belonging to different dynamical families carried out at the ESO-NTT telescope. We obtained data on 47 objects, 23 belonging to the L5 swarm and 24…

天体物理学 · 物理学 2009-11-13 S. Fornasier , E. Dotto , O. Hainaut , F. Marzari , H. Boehnhardt , F. De Luise , M. A. Barucci

We present the multi-color, five-year light curves and the first radial velocities of the near-contact binary system KR Cyg. We derived the masses of the components as 2.88$\pm$0.20 M$_{\odot}$ and 1.26$\pm$0.07 M$_{\odot}$ and the radii as…

太阳与恒星天体物理 · 物理学 2012-09-04 E. Sipahi , O. Cakirli , C. Ibanoglu

We present a comparative analysis of the spectral slope and color distributions of Jupiter Trojans, with particular attention to asteroid families. We use a sample of data from the Moving Object Catalogue of the Sloan Digital Sky Survey,…

天体物理学 · 物理学 2009-11-13 F. Roig , A. O. Ribeiro , R. Gil-Hutton