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相关论文: A Wide-Field CCD Survey for Centaurs and Kuiper Be…

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We present a survey for bright Kuiper Belt Objects (KBOs) and Centaurs, conducted at the Kitt Peak National Observatory (KPNO) 0.9 m telescope with the KPNO 8k Mosaic CCD. The survey imaged 164 sq deg near opposition to a limiting red…

天体物理学 · 物理学 2009-11-07 Chadwick A. Trujillo , Jane X. Luu , Amanda S. Bosh , James L. Elliot

The population of the Kuiper Belt within 50 AU of the Sun has likely been severely depleted by gravitational perturbations from the giant planets, particularly Neptune. The density of Kuiper Belt objects is expected to be two orders of…

天体物理学 · 物理学 2009-10-31 R. Lynne Allen , Gary Bernstein , Renu Malhotra

We present the results of a wide-field survey using the 1.2-m Samuel Oschin Telescope at Palomar Observatory. This survey was designed to find the most distant members of the Kuiper belt and beyond. We searched ~12,000 deg2 down to a mean…

地球与行星天体物理 · 物理学 2015-05-19 Megan E. Schwamb , Michael E. Brown , David L. Rabinowitz , Darin Ragozzine

We recently initiated a search for ultra-compact dwarf galaxies (UCDs) in the Centaurus galaxy cluster (Mieske et al. 2007), resulting in the discovery of 27 compact objects with -12.2<M_V<-10.9 mag. Our overall survey completeness was…

宇宙学与河外天体物理 · 物理学 2015-05-13 S. Mieske , M. Hilker , I. Misgeld , A. Jordan , L. Infante , M. Kissler-Patig

Detecting heat from minor planets in the outer solar system is challenging, yet it is the most efficient means for constraining the albedos and sizes of Kuiper Belt Objects (KBOs) and their progeny, the Centaur objects. These physical…

Almost all of the $>600$ known Kuiper belt objects (KBOs) have been discovered within 50 AU of the Sun. One possible explanation for the observed lack of KBOs beyond 50 AU is that the distant Kuiper belt is dynamically very cold, and thus…

天体物理学 · 物理学 2016-08-30 R. Lynne Allen , Gary Bernstein , Renu Malhotra

Recent stellar occultations have allowed accurate instantaneous size and apparent shape determinations of the large Kuiper belt object (50000)~Quaoar and the detection of two rings with spatially variable optical depths. In this paper we…

地球与行星天体物理 · 物理学 2024-02-22 C. Kiss , T. G. Müller , G. Marton , R. Szakáts , A. Pál , L. Molnár , E. Vilenius , M. Rengel , J. L. Ortiz , E. Fernández-Valenzuela

We conducted a search for occultations of bright stars by Kuiper Belt Objects (KBOs) to estimate the density of sub-km KBOs in the sky. We report here the first results of this occultation survey of the outer solar system conducted in June…

地球与行星天体物理 · 物理学 2011-10-27 Federica B. Bianco , Pavlos Protopapas , Brian A. McLeod , Charles R. Alcock , Matthew J. Holman , Matthew J. Lehner

Using the Max-Planck Millimeter Bolometer Array (MAMBO) at the IRAM 30m telescope we detected emission at 250 GHz from the Centaur Chariklo (1997 CU26). The observed continuum flux density implies a photometric diameter of 273 km. The…

天体物理学 · 物理学 2009-10-31 W. J. Altenhoff , K. M. Menten , F. Bertoldi

We extend previous results showing that the surfaces of Edgeworth-Kuiper Belt objects are not primordial and have been moderately to heavily reworked by collisions. Objects smaller than about $r = 2.5$ km have collisional disruption…

天体物理学 · 物理学 2009-10-31 Daniel D. Durda , S. Alan Stern

About 2500 square degrees of sky south of declination -25 degrees and/or near the galactic plane were surveyed for bright outer solar system objects. This survey is one of the first large scale southern sky and galactic plane surveys to…

Centaurs are the transitional population between trans-Neptunian objects (TNOs) and Jupiter-family comets. For this reason it is possible to access the smaller ones, which is more difficult to do with the TNO population. The goal of this…

We present the discovery of three new Scattered Kuiper Belt Objects (SKBOs) from a wide-field survey of the ecliptic. This continuing survey has to date covered 20.2 square degrees to a limiting red magnitude of 23.6. We combine the data…

天体物理学 · 物理学 2009-10-31 C. A. Trujillo , D. C. Jewitt , J. X. Luu

We have performed a survey of the Kuiper belt covering ~ 1/3 a square degree of the sky using Suprime-cam on the Subaru telescope, to a limiting magnitude of m(R)~ 26.8 (50% threshold) and have found 36 new KBOs. We have confirmed that the…

天体物理学 · 物理学 2009-11-13 W. C. Fraser , J. J. Kavelaars

We present the results of a wide-field survey for distant Sedna-like bodies in the outer solar system using the 1.2-m Samuel Oschin Telescope at Palomar Observatory. We searched ~12,000 square degrees down to a mean limiting magnitude of…

地球与行星天体物理 · 物理学 2009-11-13 Megan E. Schwamb , Michael E. Brown , David L. Rabinowitz

We describe the instrumentation and detection software and characterize the detection efficiency of an automated, all-sky, southern-hemisphere search for Kuiper Belt objects brighter than R mag 21.4. The search relies on Yale University's…

地球与行星天体物理 · 物理学 2015-06-05 David Rabinowitz , Megan E. Schwamb , Elena Hadjiyska , Suzanne Tourtellotte

We have performed an ecliptic imaging survey of the Kuiper belt with our deepest and widest field achieving a limiting flux of m(g') = 26.4, with a sky coverage of 3.0 square-degrees. This is the largest coverage of any other Kuiper belt…

We present the results of a wide-field survey designed to measure the size, inclination, and radial distributions of Kuiper Belt Objects (KBOs). The survey found 86 KBOs in 73 square degrees observed to limiting red magnitude 23.7 using the…

天体物理学 · 物理学 2009-11-06 Chadwick A. Trujillo , David C. Jewitt , Jane X. Luu

We present the results of a pencil-beam survey of the Kuiper Belt using the Keck 10-m telescope. A single 0.01 square degree field is imaged 29 times for a total integration time of 4.8 hr. Combining exposures in software allows the…

天体物理学 · 物理学 2009-10-31 E. I. Chiang , M. E. Brown
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