Search Publications

A Near-coplanar Stellar Flyby of the Planet Host Star HD 106906
DOI: 10.3847/1538-3881/ab0109 Bibcode: 2019AJ....157..125D

Kalas, Paul; De Rosa, Robert J.

We present an investigation into the kinematics of HD 106906 using the newly released Gaia DR2 catalog to search for close encounters with other members of the Scorpius-Centaurus (Sco-Cen) association. HD 106906 is an eccentric spectroscopic binary that hosts both a large asymmetric debris disk extending out to at least 500 au and a directly image…

2019 The Astronomical Journal
Gaia Hipparcos 26
ALMA Observations of Atomic Carbon [C I] ( 3 P 1 3 P 0 ) and Low-J CO Lines in the Starburst Galaxy NGC 1808
DOI: 10.3847/1538-4357/ab55dc Bibcode: 2019ApJ...887..143S

Seta, Masumichi; Salak, Dragan; Nakai, Naomasa +1 more

We present [C I] ≤ft({}3{{P}}1\to {}3{{P}}0\right), 12CO, 13CO, and C18O (J=2\to 1) observations of the central region (radius 1 kpc) of the starburst galaxy NGC 1808 at 30-50 pc resolution conducted with the Atacama Large Millimeter/submillimeter Array. Radiative transfe…

2019 The Astrophysical Journal
eHST 26
SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE
DOI: 10.1093/mnras/stz2640 Bibcode: 2019MNRAS.490.3840C

Andreani, P.; Valtchanov, I.; Clements, D. L. +21 more

We present SCUBA-2 850 µm observations of 13 candidate starbursting protoclusters selected using Planck and Herschel data. The cumulative number counts of the 850 µm sources in 9 of 13 of these candidate protoclusters show significant overdensities compared to the field, with the probability <10-2 assuming the sources are…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 26
The Precious Set of Radio-optical Reference Frame Objects in the Light of Gaia DR2 Data
DOI: 10.3847/1538-4357/aafa1c Bibcode: 2019ApJ...873..132M

Schmitt, Henrique R.; Makarov, Valeri V.; Berghea, Ciprian T. +2 more

We investigate a sample of 3413 International Celestial Reference Frame (ICRF3) extragalactic radio-loud sources with accurate positions determined by very long baseline interferometry in the S/X band, mostly active galactic nuclei and quasars, which are cross-matched with optical sources in the second Gaia data release (Gaia DR2). The main goal o…

2019 The Astrophysical Journal
Gaia 26
Alfvén Wave Propagation in the Io Plasma Torus
DOI: 10.1029/2018GL081472 Bibcode: 2019GeoRL..46.1242H

Bagenal, F.; Bonfond, B.; Hinton, P. C.

Io, the most volcanically active body in the solar system, fuels a plasma torus around Jupiter with dissociation products of SO2 at a rate of 1,000 kg/s. We use a combination of in situ Voyager 1 data and Cassini Ultraviolet Imaging Spectrograph observations to constrain a diffusive equilibrium model of the Io plasma torus. The interact…

2019 Geophysical Research Letters
eHST 26
Effects of Coronal Density and Magnetic Field Distributions on a Global Solar EUV Wave
DOI: 10.3847/1538-4357/ab2055 Bibcode: 2019ApJ...878..106H

Wang, Rui; Yang, Zhongwei; Liu, Ying D. +4 more

We investigate a global extreme-ultraviolet (EUV) wave associated with a coronal mass ejection (CME)-driven shock on 2017 September 10. The EUV wave is transmitted by north- and south-polar coronal holes (CHs), which is observed by the Solar Dynamics Observatory (SDO) and Solar Terrestrial Relations Observatory A (STEREO-A) from opposite sides of …

2019 The Astrophysical Journal
SOHO 26
Classifying exoplanet candidates with convolutional neural networks: application to the Next Generation Transit Survey
DOI: 10.1093/mnras/stz2058 Bibcode: 2019MNRAS.488.5232C

Wheatley, Peter J.; Eigmüller, Philipp; Casewell, Sarah L. +13 more

Vetting of exoplanet candidates in transit surveys is a manual process, which suffers from a large number of false positives and a lack of consistency. Previous work has shown that convolutional neural networks (CNN) provide an efficient solution to these problems. Here, we apply a CNN to classify planet candidates from the Next Generation Transit…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 26
Origin of Radio-quiet Coronal Mass Ejections in Flare Stars
DOI: 10.3847/1538-4357/ab041b Bibcode: 2019ApJ...873....1M

Mullan, D. J.; Paudel, R. R.

Type II radio bursts are observed in the Sun in association with many coronal mass ejections (CMEs). In view of this association, there has been an expectation that, by scaling from solar flares to the flares that are observed on M dwarfs, radio emission analogous to solar type II bursts should be detectable in association with M dwarf flares. How…

2019 The Astrophysical Journal
SOHO 26
VIS3COS. II. Nature and nurture in galaxy structure and morphology
DOI: 10.1051/0004-6361/201935137 Bibcode: 2019A&A...630A..57P

van der Wel, Arjen; Sobral, David; Darvish, Behnam +7 more

We study the impact of local density and stellar mass on the structure and morphology of approximately 500 quiescent and star-forming galaxies from the VIMOS Spectroscopic Survey of a Superstructure in COSMOS (VIS3COS). We perform bulge-to-disc decomposition of the surface brightness profiles and find ∼41 ± 3% of > 1010 M<…

2019 Astronomy and Astrophysics
eHST 26
Mapping the stellar age of the Milky Way bulge with the VVV. II. Deep JKs catalog release based on PSF photometry
DOI: 10.1051/0004-6361/201935730 Bibcode: 2019A&A...629A...1S

Minniti, D.; Rejkuba, M.; Zoccali, M. +6 more

Context. The bulge represents the best compromise between old and massive Galactic components, and as such its study is a valuable opportunity to understand how the bulk of the Milky Way formed and evolved. In addition, being the only bulge in which we can individually resolve stars in all evolutionary sequences, the properties of its stellar cont…

2019 Astronomy and Astrophysics
Gaia 26