Search Publications

Discovery of a Satellite of the Large Trans-Neptunian Object (225088) 2007 OR10
DOI: 10.3847/2041-8213/aa6484 Bibcode: 2017ApJ...838L...1K

Pál, András; Vinkó, József; Marton, Gábor +6 more

2007 OR10 is currently the third largest known dwarf planet in the trans-Neptunian region, with an effective radiometric diameter of ∼1535 km. It has a slow rotation period of ∼45 hr that was suspected to be caused by tidal interactions with a satellite undetected at that time. Here, we report on the discovery of a likely moon of 2007 O…

2017 The Astrophysical Journal
eHST 24
Ion-Scale Wave Properties and Enhanced Ion Heating Across the Low-Latitude Boundary Layer During Kelvin-Helmholtz Instability
DOI: 10.1002/2017JA024591 Bibcode: 2017JGRA..12211128M

Nykyri, K.; Moore, T. W.; Dimmock, A. P.

In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked solar wind. On the dawn sector, the cold-component ions are more abundant and hotter by 30-40% when compared to the dusk sector. Recent statistical studies of the flank magnetopause and magnetosheath have shown that the level of temperature asymmetr…

2017 Journal of Geophysical Research (Space Physics)
Cluster 23
Kinematics and properties of the central molecular zone as probed with [C II]
DOI: 10.1051/0004-6361/201629497 Bibcode: 2017A&A...599A.136L

Morris, M. R.; Goldsmith, P. F.; Langer, W. D. +2 more

Context. The Galactic central molecular zone (CMZ) is a region containing massive and dense molecular clouds, with dynamics driven by a variety of energy sources including a massive black hole. It is thus the nearest template for understanding physical processes in extragalactic nuclei. The CMZ's neutral interstellar gas has been mapped spectrally…

2017 Astronomy and Astrophysics
Herschel 23
The kinematic signature of the Galactic warp in Gaia DR1. I. The Hipparcos subsample
DOI: 10.1051/0004-6361/201629916 Bibcode: 2017A&A...601A.115P

Lattanzi, M. G.; Drimmel, R.; Poggio, E. +2 more

Context. The mechanism responsible for the warp of our Galaxy, as well as its dynamical nature, continues to remain unknown. With the advent of high precision astrometry, new horizons have been opened for detecting the kinematics associated with the warp and for constraining possible warp formation scenarios for the Milky Way.
Aims: The aim o…

2017 Astronomy and Astrophysics
Gaia Hipparcos 23
Tycho-Gaia Astrometric Solution Parallaxes and Proper Motions for Five Galactic Globular Clusters
DOI: 10.3847/1538-4357/aa696f Bibcode: 2017ApJ...839...89W

van der Marel, Roeland P.; Watkins, Laura L.

We present a pilot study of Galactic globular cluster (GC) proper motion (PM) determinations using Gaia data. We search for GC stars in the Tycho-Gaia Astrometric Solution (TGAS) catalog from Gaia Data Release 1 (DR1), and identify five members of NGC 104 (47 Tucanae), one member of NGC 5272 (M3), five members of NGC 6121 (M4), seven members of NG…

2017 The Astrophysical Journal
Gaia 23
Overdensities of SMGs around WISE-selected, ultraluminous, high-redshift AGNs
DOI: 10.1093/mnras/stx1141 Bibcode: 2017MNRAS.469.4565J

Tsai, Chao-Wei; Wright, Edward L.; Eisenhardt, Peter +9 more

We investigate extremely luminous dusty galaxies in the environments around Wide-field Infrared Survey Explorer (WISE)-selected hot dust-obscured galaxies (Hot DOGs) and WISE/radio-selected active galactic nuclei (AGNs) at average redshifts of z = 2.7 and 1.7, respectively. Previous observations have detected overdensities of companion submillimet…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
Toward the Understanding of the Physical Origin of Recombining Plasma in the Supernova Remnant IC 443
DOI: 10.3847/1538-4357/aa9bdf Bibcode: 2017ApJ...851...73M

Uchida, Hiroyuki; Tsuru, Takeshi Go; Tanaka, Takaaki +2 more

We perform a spatially resolved spectroscopic analysis of X-ray emission from the supernova remnant (SNR) IC 443 with Suzaku. All of the spectra are well reproduced by a model consisting of a collisional ionization equilibrium (CIE) and two recombining plasma (RP) components. Although previous X-ray studies found an RP in the northeastern region, …

2017 The Astrophysical Journal
Suzaku 23
The Solar Neighborhood. XXXX. Parallax Results from the CTIOPI 0.9 m Program: New Young Stars Near the Sun
DOI: 10.3847/1538-3881/aa8457 Bibcode: 2017AJ....154..151B

Henry, Todd J.; Winters, Jennifer G.; Jao, Wei-Chun +6 more

As a step toward completing and characterizing the census of the solar neighborhood, we present astrometric, photometric, and spectroscopic observations of 32 systems observed with the Cerro Tololo Inter-American Observatory 0.9 m and 1.5 m telescopes. Astrometry from the 0.9 m indicates that among the 17 systems that had no previous published tri…

2017 The Astronomical Journal
Gaia 23
Comparing and contrasting dispersionless injections at geosynchronous orbit during a substorm event
DOI: 10.1002/2016JA023551 Bibcode: 2017JGRA..122.3055K

Daly, P. W.; Khotyaintsev, Y.; Kozak, L. +3 more

Particle injections in the magnetosphere transport electrons and ions from the magnetotail to the radiation belts. Here we consider generation mechanisms of "dispersionless" injections, namely, those with simultaneous increase of the particle flux over a wide energy range. In this study we take advantage of multisatellite observations which simult…

2017 Journal of Geophysical Research (Space Physics)
Cluster 23
Evolution of Spin, Orbital, and Superorbital Modulations of 4U 0114+650
DOI: 10.3847/1538-4357/aa79a3 Bibcode: 2017ApJ...844...16H

Hu, Chin-Ping; Chou, Yi; Ng, C. -Y. +2 more

We report a systematic analysis of the spin, orbital, and superorbital modulations of 4U 0114+650, a high-mass X-ray binary that consists of one of the slowest spinning neutron stars. Using the dynamic power spectrum, we found that the spin period varied dramatically and is anticorrelated with the long-term X-ray flux variation that can be observe…

2017 The Astrophysical Journal
INTEGRAL 23