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Related papers: The Colors of Extreme Outer Solar System Objects

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The size distribution and total mass of objects in the Oort Cloud have important implications to the theory of planets formation, including the properties of, and the processes taking place in the early solar system. We discuss the…

Earth and Planetary Astrophysics · Physics 2015-05-14 Eran O. Ofek , Ehud Nakar

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…

Astrophysics · Physics 2009-10-28 Anita L. Cochran , Harold F. Levison , S. Alan Stern , Martin J. Duncan

We present new infrared photometry for 61 halo and disk stars around the stellar/substellar boundary. These data are combined with available optical photometry and astrometric data to produce color--color and absolute magnitude--color…

Astrophysics · Physics 2010-01-28 S. K. Leggett , F. Allard , P. H. Hauschildt

The Kuiper Belt of our solar system is a source of short-period comets that may have delivered water and other volatiles to Earth and the other terrestrial planets. However, the distribution of water and other volatiles in extrasolar…

Earth and Planetary Astrophysics · Physics 2017-02-10 S. Xu , B. Zuckerman , P. Dufour , E. D. Young , B. Klein , M. Jura

A mid-infrared (3.6-8 um) survey of the Galactic Center has been carried out with the IRAC instrument on the Spitzer Space Telescope. This survey covers the central 2x1.4 degree (~280x200 pc) of the Galaxy. At 3.6 and 4.5 um the emission is…

Only a few percent of cool, old white dwarfs (WDs) have infrared excesses interpreted as originating in small hot disks due to the infall and destruction of single asteroids that come within the star's Roche limit. Infrared excesses at 24…

Solar and Stellar Astrophysics · Physics 2015-06-19 Geoffrey C. Clayton , Orsola De Marco , Jason Nordhaus , Joel Green , Thomas Rauch , Klaus Werner , You-Hua Chu

We study the dynamical properties of objects in hyperbolic orbits passing through the inner Solar system in the context of two different potential sources: interstellar space and the Oort cloud. We analytically derive the probability…

Earth and Planetary Astrophysics · Physics 2020-01-08 Arika Higuchi , Eiichiro Kokubo

Ultra-luminous Compact X-ray Sources (ULXs) in nearby spiral galaxies and Galactic superluminal jet sources share the common spectral characteristic that they have unusually high disk temperatures which cannot be explained in the framework…

Astrophysics · Physics 2009-11-10 Ken Ebisawa , Piotr Zycki , Aya Kubota , Tsunefumi Mizuno , Ken-ya Watarai

We present the results of a search for red QSOs using a selection based on optical imaging from SDSS and near-infrared imaging from UKIDSS. For a sample of 58 candidates 46 (79%) are confirmed to be QSOs. The QSOs are predominantly…

Cosmology and Nongalactic Astrophysics · Physics 2013-01-04 J. P. U. Fynbo , J. -K. Krogager , B. Venemans , P. Noterdaeme , M. Vestergaard , P. Moller , C. Ledoux , S. Geier

We present deep color profiles for a sample of 415 disk galaxies within the redshift range 0.1<z<=1.1, and contained in HST-ACS imaging of the GOODS-South field (Giavalisco et al. 2004). For each galaxy, passband combinations are chosen to…

Astrophysics · Physics 2009-11-13 Ruyman Azzollini , Ignacio Trujillo , John E. Beckman

Outer satellites of the planets have distant, eccentric orbits that can be highly inclined or even retrograde relative to the equatorial planes of their planets. These irregular orbits cannot have formed by circumplanetary accretion and are…

Astrophysics · Physics 2009-11-11 Scott S. Sheppard

Open clusters are distributed all across the disk and are convenient tracers of its properties. In particular, outer disk clusters bear a key role for the investigation of the chemical evolution of the Galactic disk. The goal of this study…

Astrophysics of Galaxies · Physics 2016-03-30 T. Cantat-Gaudin , P. Donati , A. Vallenari , R. Sordo , A. Bragaglia , L. Magrini

We discuss the current knowledge of the Solar system, focusing on bodies in the outer regions, on the information they provide concerning Solar system formation, and on the possible relationships that may exist between our system and the…

Astrophysics · Physics 2015-05-13 David Jewitt , Amaya Moro-Martín , Pedro Lacerda

We present a new sample of 35 quasars selected from the FIRST radio survey and the Deeprange I-band survey (Postman et al. 1998, 2002). A comparison with the FIRST Bright Quasar survey samples reveals that this I-band selected sample is…

Abridged. We have performed an ecliptic survey of the Kuiper belt, with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of r'=24.7, and have detected 88 Kuiper belt objects, roughly half of which received follow-up one…

Earth and Planetary Astrophysics · Physics 2015-05-19 Wesley C. Fraser , Michael E. Brown , Megan E. Schwamb

The Deep Ecliptic Survey (DES) discovered hundreds of Kuiper Belt objects from 1998-2005. Follow-up observations yielded 304 objects with good dynamical classifications (Classical, Scattered, Centaur, or 16 mean-motion resonances with…

Earth and Planetary Astrophysics · Physics 2015-06-17 E. R. Adams , A. A. S. Gulbis , J. L. Elliot , S. D. Benecchi , M. W. Buie , D. E. Trilling , L. H. Wasserman

Several different classes of trans-Neptunian objects (TNOs) have been identified based on their optical and near-infrared colors. As part of the Colours of the Outer Solar System Origins Survey, we have obtained $g$, $r$, and $z$ band…

We present time-resolved near-infrared (J and H) photometry of the extreme Kuiper belt object (136108) Haumea (formerly 2003 EL61) taken to further investigate rotational variability of this object. The new data show that the near-infrared…

Astrophysics · Physics 2009-11-13 Pedro Lacerda

We measure the clustering of Extremely Red Objects (EROs) in ~8 deg^2 of the NOAO Deep Wide Field Survey Bo\"otes field in order to establish robust links between ERO z~1.2 and local galaxy z<0.1 populations. Three different color selection…