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Surveys of Clumps, Cores, and Condensations in Cygnus X. I. A New Catalog of ∼0.1 pc Massive Dense Cores
DOI: 10.3847/1538-4365/ab0025 Bibcode: 2019ApJS..241....1C

Qiu, Keping; Liu, Junhao; Cao, Yue +3 more

Using infrared to (sub)millimeter data from Spitzer, Herschel, the James Clerk Maxwell Telescope, and the IRAM 30 m telescope, we conducted an unbiased survey of the massive dense cores (MDCs) in the Cygnus X molecular cloud complex, aimed at characterizing the physical conditions of high-mass star formation (HMSF) at ∼0.1 pc scales. We created 5°…

2019 The Astrophysical Journal Supplement Series
Herschel 38
The velocity anisotropy of the Milky Way satellite system
DOI: 10.1093/mnras/stz973 Bibcode: 2019MNRAS.486.2679R

Grand, Robert J. J.; Gómez, Facundo A.; Fattahi, Azadeh +9 more

We analyse the orbital kinematics of the Milky Way (MW) satellite system utilizing the latest systemic proper motions for 38 satellites based on data from Gaia Data Release 2. Combining these data with distance and line-of-sight velocity measurements from the literature, we use a likelihood method to model the velocity anisotropy, β, as a function…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 38
Machine Learning Applied to Star-Galaxy-QSO Classification and Stellar Effective Temperature Regression
DOI: 10.3847/1538-3881/aaf009 Bibcode: 2019AJ....157....9B

Bai, Yu; Wang, Song; Yang, Fan +1 more

In modern astrophysics, machine learning has increasingly gained popularity with its incredibly powerful ability to make predictions or calculated suggestions for large amounts of data. We describe an application of the supervised machine-learning algorithm, random forests (RF), to the star/galaxy/QSO classification and the stellar effective tempe…

2019 The Astronomical Journal
Gaia 38
Galactic rotation from Cepheids with Gaia DR2 and effects of non-axisymmetry
DOI: 10.1093/mnras/sty2623 Bibcode: 2019MNRAS.482...40K

Bovy, Jo; Matsunaga, Noriyuki; Kawata, Daisuke +1 more

We apply a simple axisymmetric disc model to 218 Galactic Cepheids whose accurate measurements of the distance and velocities are obtained by cross-matching an existing Cepheids catalogue with the Gaia DR2 data. Our model fit determines the `local centrifugal speed', Vc - defined as the rotation speed required to balance the local radia…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 38
Particle-in-cell Simulations of Firehose Instability Driven by Bi-Kappa Electrons
DOI: 10.3847/2041-8213/ab0c95 Bibcode: 2019ApJ...873L..20L

Lazar, M.; Poedts, S.; Viñas, A. F. +4 more

We report the first results from particle-in-cell simulations of the fast-growing aperiodic electron firehose instability driven by the anisotropic bi-Kappa distributed electrons. Such electrons characterize space plasmas, e.g., solar wind and planetary magnetospheres. Predictions made by the linear theory for full wave-frequency and wave-vector s…

2019 The Astrophysical Journal
Cluster 38
H0LiCOW - X. Spectroscopic/imaging survey and galaxy-group identification around the strong gravitational lens system WFI 2033-4723
DOI: 10.1093/mnras/stz2483 Bibcode: 2019MNRAS.490..613S

Smith, M.; Annis, J.; Bertin, E. +65 more

Galaxies and galaxy groups located along the line of sight towards gravitationally lensed quasars produce high-order perturbations of the gravitational potential at the lens position. When these perturbation are too large, they can induce a systematic error on H0 of a few per cent if the lens system is used for cosmological inference an…

2019 Monthly Notices of the Royal Astronomical Society
eHST 38
SPHERE view of the jet and the envelope of RY Tauri
DOI: 10.1051/0004-6361/201935546 Bibcode: 2019A&A...628A..68G

Ménard, F.; Fantinel, D.; Podio, L. +40 more

Context. Jets are rarely associated with pre-main sequence intermediate-mass stars. This contrasts with the frequent detection of jets in lower mass or younger stars. Optical and near-IR observations of jet-driving sources are often hindered by the presence of a natal envelope.
Aims: Jets around partly embedded sources are a useful diagnostic…

2019 Astronomy and Astrophysics
Gaia 38
The Orbits of 451 Wide Visual Double Stars
DOI: 10.1134/S106377371901002X Bibcode: 2019AstL...45...30I

Izmailov, I. S.

Based on positional observations, we have determined the orbits of 130 visual double stars for the first time and improved the orbits of 321 stars. The histogram of eccentricities for all of the derived orbits corresponds to the relation f = 2e. The period distribution has two pronounced maxima at P ≈ 200 and ≈550 yr. The ephemeris relative positi…

2019 Astronomy Letters
Gaia 38
Multiple nitrogen reservoirs in a protoplanetary disk at the epoch of comet and giant planet formation
DOI: 10.1051/0004-6361/201936750 Bibcode: 2019A&A...632L..12H

Forveille, T.; Hily-Blant, P.; Magalhaes de Souza, V. +1 more

The isotopic ratio of nitrogen measured in primitive Solar System bodies shows a broad range of values, the origin of which remains unknown. One key question is whether these isotopic reservoirs of nitrogen predate the comet formation stage or are posterior to it. Another central question is elucidating the processes that can produce the observed …

2019 Astronomy and Astrophysics
Gaia 38
Li Evolution and the Open Cluster NGC 6819: A Correlation between Li Depletion and Spindown in Dwarfs More Massive Than the F-Dwarf Li-Dip
DOI: 10.3847/1538-3881/ab3fad Bibcode: 2019AJ....158..163D

Twarog, Bruce A.; Anthony-Twarog, Barbara J.; Deliyannis, Constantine P. +1 more

Spectroscopy of 333 NGC 6819 stars and Gaia astrometry are used to map Li evolution from the giant branch tip to 0.5 mag below the Li dip. Isochrone comparison with [Fe/H] = -0.04, based upon neural network spectroscopic analysis, produces an age of 2.25 (2.4) Gyr for E(B - V) = 0.16 (0.14) and (m - M) = 12.40 (12.29). Despite originating outside …

2019 The Astronomical Journal
Gaia 38