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Eigenfunctions of Galactic phase space spirals from dynamic mode decomposition
DOI: 10.1093/mnras/stz2539 Bibcode: 2019MNRAS.490..114D

Widrow, Lawrence M.; Darling, Keir

We investigate the spatiotemporal structure of simulations of the homogeneous slab and isothermal plane models for the vertical motion in the Galactic disc. We use dynamic mode decomposition (DMD) to compute eigenfunctions of the simulated distribution functions for both models, referred to as DMD modes. In the case of the homogeneous slab, we com…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 17
K2-161b: a low-density super-Neptune on an eccentric orbit
DOI: 10.1093/mnras/sty3230 Bibcode: 2019MNRAS.483.1970B

Jones, M. I.; Cortés, C.; Rabus, M. +15 more

We report the discovery of K2-161b, which was first identified as a planetary candidate from Kepler K2 photometry of Campaign 14, and whose planetary nature and orbital parameters were then confirmed with precision radial velocities. K2-161b is half as massive as Saturn (M_P= 0.179 ± 0.021 MJ), and has a radius of R_P= 0.840 ± 0.011 R_J…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 17
WASP-180Ab: Doppler tomography of a hot Jupiter orbiting the primary star in a visual binary
DOI: 10.1093/mnras/stz2632 Bibcode: 2019MNRAS.490.2467T

Bouchy, F.; Queloz, D.; Ségransan, D. +26 more

We report the discovery and characterization of WASP-180Ab, a hot Jupiter confirmed by the detection of its Doppler shadow and by measuring its mass using radial velocities. We find the 0.9 ± 0.1 MJup, 1.24 ± 0.04 RJup planet to be in a misaligned, retrograde orbit around an F7 star with Teff = 6500 K and a moderat…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 17
Studying the physical properties of tidal features - I. Extracting morphological substructure in CANDELS observations and VELA simulations
DOI: 10.1093/mnras/stz872 Bibcode: 2019MNRAS.486.2643M

Bell, Eric F.; Ferguson, Henry C.; Hathi, Nimish P. +17 more

The role of major mergers in galaxy evolution remains a key open question. Existing empirical merger identification methods use non-parametric and subjective visual classifications that can pose systematic challenges to constraining merger histories. As a first step towards overcoming these challenges, we develop and share publicly a new PYTHON-ba…

2019 Monthly Notices of the Royal Astronomical Society
eHST 17
The tale of the Milky Way globular cluster NGC 6362 - I. The orbit and its possible extended star debris features as revealed by Gaia DR2
DOI: 10.1093/mnras/stz2500 Bibcode: 2019MNRAS.489.4565K

Robin, Annie C.; Minniti, Dante; Fernández-Trincado, José G. +5 more

We report the identification of possible extended star debris candidates beyond the cluster tidal radius of NGC 6362 based on the second Gaia data release (Gaia DR2). We found 259 objects possibly associated with the cluster lying in the vicinity of the giant branch and 1-2 magnitudes fainter/brighter than the main-sequence turn-off in the cluster…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 17
Spectroscopic and astrometric radial velocities: Hyades as a benchmark
DOI: 10.1093/mnras/sty3215 Bibcode: 2019MNRAS.483.5026L

Pasquini, L.; Ludwig, H. -G.; de Medeiros, J. R. +1 more

We study the accuracy of spectroscopic radial velocities (RVs) by comparing spectroscopic and astrometric RVs for stars of the Hyades open cluster. We obtained High-Accuracy Radial velocity Planet Searcher (HARPS) spectra for a large sample of Hyades stars and combined them with accurate astrometric RVs based on Hipparcos and Gaia data. After clea…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 17
Resolving accretion flows in nearby active galactic nuclei with the Event Horizon Telescope
DOI: 10.1093/mnras/stz2874 Bibcode: 2019MNRAS.490.4606B

Nagar, Neil M.; Ramakrishnan, Venkatessh; Xie, Fu-Guo +5 more

The Event Horizon Telescope (EHT), now with its first ever image of the photon ring around the supermassive black hole of M87, provides a unique opportunity to probe the physics of supermassive black holes through Very Long Baseline Interferometry (VLBI), such as the existence of the event horizon, the accretion processes as well as jet formation …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 17
GJ 357: a low-mass planetary system uncovered by precision radial velocities and dynamical simulations
DOI: 10.1093/mnras/stz2937 Bibcode: 2019MNRAS.490.5585J

Suárez, Juan C.; Tuomi, M.; Jenkins, J. S. +5 more

We report the detection of a new planetary system orbiting the nearby M2.5V star GJ 357, using precision radial velocities from three separate echelle spectrographs, High Accuracy Radial velocity Planet Searcher (HARPS), High Resolution Echelle Spectrograph (HiRES), and Ultraviolet and Visible Echelle Spectrograph (UVES). Three small planets have …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 17
The central star of planetary nebula PHR 1315 - 6555 and its host Galactic open cluster AL 1
DOI: 10.1093/mnras/stz108 Bibcode: 2019MNRAS.484.3078F

Lykou, F.; Zijlstra, A.; Parker, Q. A. +2 more

PHR 1315 - 6555 is a rare case of a Galactic planetary nebula that is a proven member of the open cluster AL 1. This membership allows its distance to be defined with precision, and thus accurate measurements of its physical characteristics along with the parameters of its central star (CS) can be obtained. In this work, we use the Hubble Space Te…

2019 Monthly Notices of the Royal Astronomical Society
eHST 17
Multi-epoch X-ray spectral analysis of the narrow-line Seyfert 1 galaxy Mrk 478
DOI: 10.1093/mnras/stz2518 Bibcode: 2019MNRAS.489.5398W

Gallo, L. C.; Zoghbi, A.; Gonzalez, A. G. +2 more

A multi-epoch X-ray spectral and variability analysis is conducted for the narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) Mrk 478. All available X-ray data from XMM-Newton and Suzaku satellites, spanning from 2001 to 2017, are modelled with a variety of physical models, including partial covering, soft Comptonization, and blurred refle…

2019 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 17