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

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One of the most striking and curious features of the small Kuiper Belt Object (KB), Arrokoth, explored by New Horizons, is the bright, annular neck it exhibits at the junction between its two lobes. Here we summarize past reported findings…

地球与行星天体物理 · 物理学 2021-03-22 S. Alan Stern , Brian Keeney , Kelsi Singer , Oliver White , Jason D. Hofgartner , Will Grundy , The New Horizons Team

We have started since 1997 the Meudon Multicolor Survey of Outer Solar System Objects with the aim of collecting a large and homogeneous set of color data for Trans-Neptunian and Centaurs objects [...] We have a combined sample of 52 B-R…

天体物理学 · 物理学 2009-11-07 A. Doressoundiram , N. Peixinho , C. de Bergh , S. Fornasier , Ph. Thebault , M. A. Barucci , C. Veillet

The Next Generation Virgo Cluster Survey is a 104 square degree survey of the Virgo Cluster, carried out using the MegaPrime camera of the Canada-France-Hawaii telescope, from semesters 2009A-2012A. The survey will provide coverage of this…

宇宙学与河外天体物理 · 物理学 2015-05-30 Nicholas M. Ball

Scorpius-Centaurus is the nearest OB association and its hundreds of members were divided into sub-groups, including Lower Centaurus Crux. Here we study the dynamics of the Lower Centaurus Crux area stellar content. We report the revelation…

太阳与恒星天体物理 · 物理学 2018-11-28 Bertrand Goldman , Siegfried Roeser , Elena Schilbach , Attila C. Moór , Thomas Henning

We present the data acquisition strategy and characterization procedures for the Canada-France Ecliptic Plane Survey (CFEPS), a sub-component of the Canada-France-Hawaii Telescope Legacy Survey. The survey began in early 2003 and as of…

Knowledge of the Kuiper Belt is currently limited to those objects that can be detected directly. Objects with diameters less than $\sim$10km reflect too little light to be detected. These smaller bodies could contain most of the mass in…

天体物理学 · 物理学 2007-12-11 R. Stevenson

The centaur (2060) Chiron has exhibited outgassing behaviour and possibly hosts a ring system. On 2011 November 29, Chiron occulted a fairly bright star (R approximately 15 mag) as observed from the 3-m NASA Infrared Telescope Facility…

地球与行星天体物理 · 物理学 2020-01-08 A. A. Sickafoose , A. S. Bosh , J. P. Emery , M. J. Person , C. A. Zuluaga , M. Womack , J. D. Ruprecht , F. B. Bianco , A. M. Zangari

Context: Alpha Centauri is our closest stellar neighbor, at a distance of only 1.3 pc, and its two main components have spectral types comparable to the Sun. This is therefore a favorable target for an imaging search for extrasolar planets.…

Bright high-redshift quasars ($z>6$), hosting supermassive black holes ($\rm M_{BH} > 10^8 M_{\odot}$), are expected to reside in massive host galaxies embedded within some of the earliest and most massive galaxy overdensities. We analyze…

We report on the results of infrared spectroscopic mapping observations carried out in the nuclear region of Centaurus A (NGC5128). The 500 pc bipolar dust shell discovered by Quillen et al.(2006) is even more clearly seen in the 11.3…

A stellar occultation of Gaia DR3 2646598228351156352 by the Centaur (2060) Chiron was observed from the South African Astronomical Observatory on 2018 November 28 UT. Here we present a positive detection of material surrounding Chiron from…

We present theoretical constraints for the formation of the newly discovered dark star clusters (DSCs) with high mass-to-light (M/L) ratios, from Taylor et al (2015). These compact stellar systems photometrically resemble globular clusters…

星系天体物理 · 物理学 2016-12-07 Mia Sauda Bovill , Thomas H. Puzia , Massimo Ricotti , Matthew A. Taylor

We present analysis of {\it Hubble Space Telescope} (HST) observations of Centaur 29P/Schwassmann-Wachmann 1 (SW1) while in outburst to characterize the outburst coma and place constraints on the nucleus' spin state. The observations…

地球与行星天体物理 · 物理学 2020-01-08 Charles Schambeau , Yanga Fernandez , Nalin Samarasinha , Laura Woodney , Arunav Kundu

We present differential radial velocity measurements of Proxima Centauri collected over 4 years with the ESO CES with a mean precision of $54 ms^{-1}$. We find no evidence of a periodic signal that could corroborate the existence of a…

天体物理学 · 物理学 2011-05-23 M. Kürster , A. P. Hatzes , W. D. Cochran , S. Döbereiner , K. Dennerl , M. Endl

New large-scale CO surveys of the first and second Galactic quadrants and the nearby molecular cloud complexes in Orion and Taurus, obtained with the CfA 1.2 m telescope, have been combined with 31 other surveys obtained over the past two…

天体物理学 · 物理学 2009-10-31 T. M. Dame , Dap Hartmann , P. Thaddeus

We report the results of 20, 6, and 2 cm VLA and 1.5 cm OVRO observations of the optically-selected CfA Seyfert galaxies and the bolometric-flux-limited 12-Micron active galaxy sample. Every object observed was detected at 6 cm. Only 6-8%…

天体物理学 · 物理学 2009-10-28 Brian Rush , Matthew A. Malkan , Richard A. Edelson

We report 250 GHz (1.2mm) observations of redshift > 3.8 quasars from the Palomar Sky Survey (PSS) sample, using the Max-Planck Millimetre Bolometer (MAMBO) array at the IRAM 30-metre telescope. Eighteen sources were detected and upper…

天体物理学 · 物理学 2009-11-06 A. Omont , P. Cox , F. Bertoldi , R. G. McMahon , C. Carilli , K. G. Isaak

Images of the Kuiper belt object (126719) 2002 CC249 obtained in 2016 and 2017 using the 6.5m Magellan-Baade Telescope and the 4.3m Discovery Channel Telescope are presented. A lightcurve with a periodicity of 11.87+/-0.01 h and a…

地球与行星天体物理 · 物理学 2017-12-06 Audrey Thirouin , Scott S. Sheppard

To prepare for the upcoming Legacy Survey of Space and Time, we develop methods for quantifying the selection function of a wide-field survey as a function of all six orbital parameters and absolute magnitude. We perform a HelioLinC3D…

地球与行星天体物理 · 物理学 2024-12-03 Jacob A. Kurlander , Matthew J. Holman , Pedro H. Bernardinelli , Mario Juric , Aren N. Heinze , Matthew J. Payne

We present an imaging survey aimed at searching for the stellar counterparts of recently discovered ultra-compact high-velocity HI clouds (UCHVC). Adams et al. (2013) proposed these clouds to be candidate mini-haloes in the Local Group…

星系天体物理 · 物理学 2015-06-23 M. Bellazzini , G. Beccari , G. Battaglia , N. Martin , V. Testa , R. Ibata , M. Correnti , F. Cusano , E. Sani