Search Publications

Jupiter's ammonia distribution derived from VLA maps at 3-37 GHz
DOI: 10.1016/j.icarus.2018.11.024 Bibcode: 2019Icar..322..168D

de Pater, Imke; Sault, R. J.; Wong, Michael H. +3 more

We observed Jupiter four times over a full rotation (10 h) with the upgraded Karl G. Jansky Very Large Array (VLA) between December 2013 and December 2014. Preliminary results at 4-17 GHz were presented in de Pater et al. (2016); in the present paper we present the full data set at frequencies between 3 and 37 GHz. Major findings are:

i) The …

2019 Icarus
eHST 50
Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2. II. Resolved common proper motion pairs
DOI: 10.1051/0004-6361/201834211 Bibcode: 2019A&A...623A.117K

Mérand, Antoine; Evans, Nancy Remage; Gieren, Wolfgang +6 more

Context. The multiplicity of classical Cepheids (CCs) and RR Lyrae stars (RRLs) is still imperfectly known, particularly for RRLs.
Aims: In order to complement the close-in short orbital period systems presented in Paper I, our aim is to detect the wide, spatially resolved companions of the targets of our reference samples of Galactic CCs and…

2019 Astronomy and Astrophysics
Gaia 50
The age of the Galactic stellar halo from Gaia white dwarfs
DOI: 10.1093/mnras/sty2755 Bibcode: 2019MNRAS.482..965K

Hambly, N. C.; Rowell, N.; Bergeron, P. +3 more

We use 156 044 white dwarf candidates with ≥5σ significant parallax measurements from the Gaia mission to measure the velocity dispersion of the Galactic disc; (σU, σV, σW) = (30.8, 23.9, 20.0) km s-1. We identify 142 objects that are inconsistent with disc membership at the >5σ level. This is the lar…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 50
The role of molecular filaments in the origin of the prestellar core mass function and stellar initial mass function
DOI: 10.1051/0004-6361/201935915 Bibcode: 2019A&A...629L...4A

André, Ph.; Arzoumanian, D.; Könyves, V. +2 more

Context. The origin of the stellar initial mass function (IMF) is one of the most debated issues in astrophysics.
Aims: Here we explore the possible link between the quasi-universal filamentary structure of star-forming molecular clouds and the origin of the IMF.
Methods: Based on our recent comprehensive study of filament properties fro…

2019 Astronomy and Astrophysics
Herschel 50
The Evolution of the He II-ionizing Background at Redshifts 2.3 < z < 3.8 Inferred from a Statistical Sample of 24 HST/COS He II Lyα Absorption Spectra
DOI: 10.3847/1538-4357/ab0fa1 Bibcode: 2019ApJ...875..111W

Hennawi, Joseph F.; Worseck, Gábor; Prochaska, J. Xavier +1 more

We present measurements of the large-scale (≈40 comoving Mpc) effective optical depth of He II Lyα absorption, {τ }eff}, at 2.54 < z < 3.86 toward 16 He II-transparent quasars observed with the Cosmic Origins Spectrograph on the Hubble Space Telescope, to characterize the ionization state of helium in the intergalactic medium (IGM…

2019 The Astrophysical Journal
eHST 50
Kinematics with Gaia DR2: the force of a dwarf
DOI: 10.1093/mnras/stz2343 Bibcode: 2019MNRAS.490..797C

Anders, F.; Chiappini, C.; Santiago, B. X. +10 more

We use Gaia DR2 astrometric and line-of-sight velocity information combined with two sets of distances obtained with a Bayesian inference method to study the 3D velocity distribution in the Milky Way disc. We search for variations in all Galactocentric cylindrical velocity components (Vϕ, VR, and Vz) with Galactic …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 50
New Constraints on the Nuclear Equation of State from the Thermal Emission of Neutron Stars in Quiescent Low-mass X-Ray Binaries
DOI: 10.3847/1538-4357/ab4f6c Bibcode: 2019ApJ...887...48B

Guillot, Sebastien; Webb, Natalie; Reisenegger, Andreas +3 more

This paper presents a new analysis of the thermal emission from the neutron star (NS) surface to constrain the dense matter equation of state. We employ an empirical parameterization of the equation of state with a Markov Chain Monte Carlo approach to consistently fit the spectra of quiescent low-mass X-ray binaries in globular clusters with well-…

2019 The Astrophysical Journal
Gaia XMM-Newton 50
On the Mass Accretion Rate and Infrared Excess in Herbig Ae/Be Stars
DOI: 10.3847/1538-3881/ab0ca1 Bibcode: 2019AJ....157..159A

Arun, R.; Mathew, Blesson; Manoj, P. +5 more

The present study makes use of the unprecedented capability of the Gaia mission to obtain the stellar parameters such as distance, age, and mass of HAeBe stars. The accuracy of Gaia DR2 astrometry is demonstrated from the comparison of the Gaia DR2 distances of 131 HAeBe stars with the previously estimated values from the literature. This is one o…

2019 The Astronomical Journal
Gaia 50
Universality of Lower Hybrid Waves at Earth's Magnetopause
DOI: 10.1029/2019JA027155 Bibcode: 2019JGRA..124.8727G

Lavraud, B.; Génot, V.; André, M. +15 more

Waves around the lower hybrid frequency are frequently observed at Earth's magnetopause and readily reach very large amplitudes. Determining the properties of lower hybrid waves is crucial because they are thought to contribute to electron and ion heating, cross-field particle diffusion, anomalous resistivity, and energy transfer between electrons…

2019 Journal of Geophysical Research (Space Physics)
Cluster 50
Gaia GraL: Gaia DR2 Gravitational Lens Systems. III. A systematic blind search for new lensed systems
DOI: 10.1051/0004-6361/201833802 Bibcode: 2019A&A...622A.165D

Djorgovski, S. G.; Stern, D.; Surdej, J. +13 more


Aims: In this work, we aim to provide a reliable list of gravitational lens candidates based on a search performed over the entire Gaia Data Release 2 (Gaia DR2). We also aim to show that the astrometric and photometric information coming from the Gaia satellite yield sufficient insights for supervised learning methods to automatically identi…

2019 Astronomy and Astrophysics
Gaia 50