Search Publications

New Substellar Discoveries from Kepler and K2: Is There a Brown Dwarf Desert?
DOI: 10.3847/1538-3881/ab245e Bibcode: 2019AJ....158...38C

Latham, David W.; Carmichael, Theron W.; Vanderburg, Andrew M.

We present the discoveries of a brown dwarf (BD) and a low-mass star from the Kepler and K2 missions. The newly discovered BD is EPIC 212036875b and the low-mass star is KOI-607b. EPIC 212036875b has a mass of M b = 52.3 ± 1.9 M J, a radius of R b = 0.874 ± 0.017 R J, and orbits its host star in P = …

2019 The Astronomical Journal
Gaia 31
Formation of globular cluster systems - II. Impact of the cut-off of the cluster initial mass function
DOI: 10.1093/mnras/stz811 Bibcode: 2019MNRAS.486..331C

Gnedin, Oleg Y.; Choksi, Nick

Observations of young star clusters reveal that the high-mass end of the cluster initial mass function (CIMF) deviates from a pure power law and instead truncates exponentially. We investigate the effects of this truncation on the formation of globular cluster (GC) systems by updating our analytic model for cluster formation and evolution, which i…

2019 Monthly Notices of the Royal Astronomical Society
eHST 31
Ultra-bright CO and [C I] Emission in a Lensed z = 2.04 Submillimeter Galaxy with Extreme Molecular Gas Properties
DOI: 10.3847/1538-3881/aaf50b Bibcode: 2019AJ....158...34D

Rebolo, R.; Krips, M.; Dannerbauer, H. +4 more

We report the very bright detection of cold molecular gas with the IRAM NOEMA interferometer of the strongly lensed source WISE J132934.18+224327.3 at z = 2.04, the so-called Cosmic Eyebrow. This source has a similar spectral energy distribution from optical-mid/IR to submillimeter/radio but significantly higher fluxes than the well-known lensed S…

2019 The Astronomical Journal
eHST 31
Observational Analysis on the Early Evolution of a CME Flux Rope: Preflare Reconnection and Flux Rope’s Footpoint Drift
DOI: 10.3847/1538-4357/ab527e Bibcode: 2019ApJ...887..118C

Yang, Jiayan; Ji, Kaifan; Duan, Yadan +1 more

We study the early evolution of a hot-channel-like magnetic flux rope (MFR) toward eruption. Combining with imaging observation and magnetic field extrapolation, we find that the hot channel possibly originated from a preexisting seed MFR with a hyperbolic flux tube (HFT). In the precursor phase, three-dimensional tether-cutting reconnection at th…

2019 The Astrophysical Journal
SOHO 31
Dust properties and star formation of approximately a thousand local galaxies
DOI: 10.1051/0004-6361/201834553 Bibcode: 2019A&A...631A..38L

Barmby, P.; Lehnert, M.; Lianou, S. +2 more


Aims: We derived the dust properties for 753 local galaxies and examine how these relate to some of their physical properties. We present the derived dust emission properties, including model spectral energy distribution (SEDs), star formation rates (SFRs) and stellar masses, as well as their relations.
Methods: We modelled the global du…

2019 Astronomy and Astrophysics
Herschel 31
X-ray spectra of the Fe-L complex
DOI: 10.1051/0004-6361/201833860 Bibcode: 2019A&A...627A..51G

Raassen, A. J. J.; Gu, Liyi; Mao, Junjie +7 more

The Hitomi results on the Perseus cluster have led to improvements in our knowledge of atomic physics that are crucial for the precise diagnostic of hot astrophysical plasma observed with high-resolution X-ray spectrometers. However, modeling uncertainties remains, both within but especially beyond Hitomi's spectral window. A major challenge in sp…

2019 Astronomy and Astrophysics
XMM-Newton 31
The scattered disc of HR 8799
DOI: 10.1093/mnras/sty3160 Bibcode: 2019MNRAS.483..332G

Booth, Mark; Krivov, Alexander V.; Löhne, Torsten +1 more

HR 8799 is a young F0-type star with four directly imaged giant planets and two debris belts, one located exterior and another one interior to the region occupied by the planetary orbits. Not only having an architecture similar to that of our Solar system but also revealing dissimilarities such as high masses of planets, a huge radial extent, and …

2019 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 31
The Formation Conditions of the Wide Binary Class 0 Protostars within BHR 71
DOI: 10.3847/1538-4357/aaef87 Bibcode: 2019ApJ...870...81T

Bourke, Tyler L.; Codella, Claudio; Chen, Xuepeng +7 more

We present a characterization of the binary protostar system that is forming within a dense core in the isolated dark cloud BHR71. The pair of protostars, IRS1 and IRS2, are both in the Class 0 phase, determined from observations that resolve the sources from 1 µm out to 250 µm and from 1.3 mm to 1.3 cm. The resolved observations enabl…

2019 The Astrophysical Journal
Herschel 31
Testing dark matter with Cherenkov light — prospects of H.E.S.S. and CTA for exploring minimal supersymmetry
DOI: 10.1007/JHEP10(2019)043 Bibcode: 2019JHEP...10..043H

Moulin, Emmanuel; Hryczuk, Andrzej; Jodłowski, Krzysztof +4 more

We provide an updated and improved study of the prospects of the H.E.S.S. and Cherenkov Telescope Array (CTA) experiments in testing neutralino dark matter in the Minimal Supersymmetric Standard Model with nine free parameters (p9MSSM). We include all relevant experimental constraints and theoretical developments, in particular a calculation of th…

2019 Journal of High Energy Physics
Gaia 31
Gas velocity structure of the Orion A integral-shaped filament
DOI: 10.1093/mnras/stz2512 Bibcode: 2019MNRAS.489.4771G

Stutz, Amelia M.; González Lobos, Vale

We present analysis of the gas kinematics of the integral-shaped filament (ISF) in Orion A using four different molecular lines, 12CO (1-0), 13CO (1-0), NH3 (1,1), and N2H+ (1-0). We describe our method to visualize the position-velocity (PV) structure using the intensity-weighted line velocit…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 31