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

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Occultations provide indirect sensitivity to the number density of small Kuiper Belt objects (KBOs) too faint to directly detect telescopically. We present results from the Caltech HI-speed Multicolor camERA (CHIMERA) survey with the…

地球与行星天体物理 · 物理学 2023-11-17 Qicheng Zhang , Gregg W. Hallinan , Navtej S. Saini , Hilke E. Schlichting , Leon K. Harding , Jennifer W. Milburn

Proxima Centauri, the star closest to our Sun, is known to host at least one terrestrial planet candidate in a temperate orbit. Here we report the ALMA detection of the star at 1.3 mm wavelength and the discovery of a belt of dust orbiting…

Centaurs are solar system objects with orbits situated among the orbits of Jupiter and Neptune. Centaurs represent one of the sources of Near-Earth Objects. Thus, it is crucial to understand their orbital evolution which in some cases might…

地球与行星天体物理 · 物理学 2018-10-17 M. A. Galiazzo , E. A. Silber , R. Dvorak

We propose a Roman Space Telescope survey to investigate fundamental properties of the distant solar system in the region of the Kuiper Belt where object characteristics and the size distribution are inaccessible from any other telescope.…

This paper presents the first results of a survey for bright quasars (V < 14.5 and R<15.4) covering the North Hemisphere at galactic latitudes |b|>30. The photometric database is derived from the GSC and USNO catalogs. Quasars are…

天体物理学 · 物理学 2009-10-31 A. Grazian , S. Cristiani , V. D'Odorico , A. Omizzolo , A. Pizzella

The DECam Ecliptic Exploration Project (DEEP) is a deep survey of the trans-Neptunian solar system being carried out on the 4-meter Blanco telescope at Cerro Tololo Inter-American Observatory in Chile using the Dark Energy Camera (DECam).…

We present time series photometry of Bienor in four observation campaigns from 2013 to 2016 and compare them with previous observations in the literature dating back to 2000. The results show a remarkable decline in the amplitude of the…

地球与行星天体物理 · 物理学 2017-04-19 E. Fernández-Valenzuela , J. L. Ortiz , R. Duffard , N. Morales , P. Santos-Sanz

We present the widest-field resolved stellar map to date of the closest ($D\sim3.8$ Mpc) massive elliptical galaxy NGC 5128 (Centaurus A; Cen A), extending out to a projected galactocentric radius of $\sim150$ kpc. The dataset is part of…

星系天体物理 · 物理学 2016-05-25 D. Crnojević , D. J. Sand , K. Spekkens , N. Caldwell , P. Guhathakurta , B. McLeod , A. Seth , J. Simon , J. Strader , E. Toloba

The Kuiper belt object Orcus and its satellite Vanth form an unusual system in the Kuiper belt. Orcus is amongst the largest objects known in the Kuiper belt, but the relative size of Vanth is much larger than that of the tiny satellites of…

地球与行星天体物理 · 物理学 2015-05-14 M. E. Brown , D. Ragozzine , J. Stansberry , W. C. Fraser

Centaurs have orbits between Jupiter and Neptune and are thought to originate from the trans-Neptunian region. Observations of surface properties of Centaurs and comparison with those of trans-Neptunian objects (TNOs) would provide…

地球与行星天体物理 · 物理学 2018-11-28 Haruka Sakugawa , Tsuyoshi Terai , Keiji Ohtsuki , Fumi Yoshida , Naruhisa Takato , Patryk Sofia Lykawka , Shiang-Yu Wang

Measuring the size distribution of small (km-scale) KBOs can help constrain models of Solar System formation and planetary migration. Such small, distant bodies are hard to detect with current or planned telescopes, but can be identified as…

地球与行星天体物理 · 物理学 2023-10-06 Guy Nir , Eran O. Ofek , David Polishook , Barak Zackay , Sagi Ben-Ami

We present results from X-ray observations of the quadruply lensed quasar RX J0911.4+0551 using data obtained with the Advanced CCD Imaging Spectrometer (ACIS) on board the Chandra X-ray Observatory. The 29 ks observation detects a total of…

The recent discovery of an earth-like planet around Proxima Centauri has drawn much attention to this star and its environment. We performed a series of observations of Proxima Centauri using SPHERE, the planet finder instrument installed…

The mass M, and the radius R_h, of the Centaurus A group are estimated from the positions and radial velocities of 30 probable cluster members. For an assumed distance of 3.9 Mpc it is found that R_h \sim 640 kpc. The velocity dispersion in…

天体物理学 · 物理学 2009-10-31 Sidney van den Bergh

We have measured the mid-infrared thermal continua from two Centaurs, inactive (8405) Asbolus and active 95P=(2060) Chiron, and have constrained their geometric albedos, p, and effective radii, R, with the Standard Thermal Model for slow…

天体物理学 · 物理学 2009-11-07 Y. R. Fernandez , D. C. Jewitt , S. S. Sheppard

Most comets are volatile-rich bodies that have recently entered the inner solar system following long-term storage in the Kuiper belt and the Oort cloud reservoirs. These reservoirs feed several distinct, short-lived "small body"…

地球与行星天体物理 · 物理学 2015-12-23 Dave Jewitt

We report the statistical detection (at the >99% confidence level) of a population of 28th magnitude objects exhibiting proper motions of ~1 arcsecond per hour at quadrature in deep HST/WFPC2 images. The drift directions imply a…

天体物理学 · 物理学 2009-10-28 Anita L. Cochran , Harold F. Levison , S. Alan Stern , Martin J. Duncan

We describe the discovery of a bright, young Kuiper belt-like debris disk around HD 115600, a $\sim$ 1.4--1.5 M$_\mathrm{\odot}$, $\sim$ 15 Myr old member of the Sco-Cen OB Association. Our H-band coronagraphy/integral field spectroscopy…

Using the absolute detection calibration and abundant detections of the OSSOS (Outer Solar System Origin Survey) project, we provide population measurements for the main Kuiper Belt. For absolute magnitude $H_r<8.3$, there are 30,000…

地球与行星天体物理 · 物理学 2023-09-06 Jean-Marc Petit , Brett Gladman , J. J. Kavelaars , Michele T. Bannister , Mike Alexandersen , Kathryn Volk , Ying-Tung Chen

We present I-band Surface Brightness Fluctuations (SBF) measurements for 16 early type galaxies (3 giants, 13 dwarfs) in the central region of the Hydra cluster, based on deep photometric data in 7 fields obtained with VLT FORS1. From the…

天体物理学 · 物理学 2009-11-10 S. Mieske , M. Hilker , L. Infante