Search Publications

Non-LTE chemical abundances in Galactic open and globular clusters
DOI: 10.1051/0004-6361/201935861 Bibcode: 2019A&A...628A..54K

Ting, Yuan-Sen; Kovalev, Mikhail; Rix, Hans-Walter +1 more


Aims: We study the effects of non-local thermodynamic equilibrium (NLTE) on the determination of stellar parameters and abundances of Fe, Mg, and Ti from the medium-resolution spectra of FGK stars.
Methods: We extended the Payne fitting approach to draw on NLTE and LTE spectral models. These were used to analyse the spectra of the Gaia-E…

2019 Astronomy and Astrophysics
Gaia 55
Stringent limits on the magnetic field strength in the disc of TW Hya. ALMA observations of CN polarisation
DOI: 10.1051/0004-6361/201935459 Bibcode: 2019A&A...624L...7V

Testi, L.; Williams, J. P.; Facchini, S. +8 more

Despite their importance in the star formation process, measurements of magnetic field strength in proto-planetary discs remain rare. While linear polarisation of dust and molecular lines can give insight into the magnetic field structure, only observations of the circular polarisation produced by Zeeman splitting provide a direct measurement of m…

2019 Astronomy and Astrophysics
Gaia 55
Spatial segregation of dust grains in transition disks. SPHERE observations of 2MASS J16083070-3828268 and RXJ1852.3-3700
DOI: 10.1051/0004-6361/201834800 Bibcode: 2019A&A...624A...7V

Pinte, C.; Ménard, F.; Dent, W. R. F. +27 more

Context. The mechanisms governing the opening of cavities in transition disks are not fully understood. Several processes have been proposed, but their occurrence rate is still unknown.
Aims: We present spatially resolved observations of two transition disks, and aim at constraining their vertical and radial structure using multiwavelength ob…

2019 Astronomy and Astrophysics
Gaia 54
Blobs, spiral arms, and a possible planet around HD 169142
DOI: 10.1051/0004-6361/201834760 Bibcode: 2019A&A...623A.140G

Henning, T.; Fantinel, D.; D'Orazi, V. +24 more

Context. Young planets are expected to cause cavities, spirals, and kinematic perturbations in protostellar disks that may be used to infer their presence. However, a clear detection of still-forming planets embedded within gas-rich disks is still rare.
Aims: HD 169142 is a very young Herbig Ae-Be star surrounded by a pre-transitional disk, c…

2019 Astronomy and Astrophysics
Gaia 54
Star-forming content of the giant molecular filaments in the Milky Way
DOI: 10.1051/0004-6361/201732400 Bibcode: 2019A&A...622A..52Z

Henning, Th.; Zhang, M.; Fang, M. +2 more

Context. Through observations numerous giant molecular filaments (GMFs) have been discovered in the Milky Way. Their role in the Galactic star formation and Galaxy-scale evolution of dense gas is unknown.
Aims: We investigate systematically the star-forming content of all currently known GMFs. This allows us to estimate the star formation rat…

2019 Astronomy and Astrophysics
Herschel 53
Euclid preparation. IV. Impact of undetected galaxies on weak-lensing shear measurements
DOI: 10.1051/0004-6361/201935187 Bibcode: 2019A&A...627A..59E

Lilje, P. B.; Scott, D.; Schrabback, T. +22 more

In modern weak-lensing surveys, the common approach to correct for residual systematic biases in the shear is to calibrate shape measurement algorithms using simulations. These simulations must fully capture the complexity of the observations to avoid introducing any additional bias. In this paper we study the importance of faint galaxies below th…

2019 Astronomy and Astrophysics
eHST 53
Confirmation of the radial velocity super-Earth K2-18c with HARPS and CARMENES
DOI: 10.1051/0004-6361/201833995 Bibcode: 2019A&A...621A..49C

Bouchy, F.; Doyon, R.; Bonfils, X. +13 more

In an earlier campaign to characterize the mass of the transiting temperate super-Earth K2-18b with HARPS, a second, non-transiting planet was posited to exist in the system at 9 days. Further radial velocity follow-up with the CARMENES spectrograph visible channel revealed a much weaker signal at 9 days, which also appeared to vary chromatically …

2019 Astronomy and Astrophysics
Gaia 53
Rotation rate of the solar core as a key constraint to magnetic angular momentum transport in stellar interiors
DOI: 10.1051/0004-6361/201935509 Bibcode: 2019A&A...626L...1E

Buldgen, G.; Eggenberger, P.; Salmon, S. J. A. J.

Context. The internal rotation of the Sun constitutes a fundamental constraint when modelling angular momentum transport in stellar interiors. In addition to the more external regions of the solar radiative zone probed by pressure modes, measurements of rotational splittings of gravity modes would offer an invaluable constraint on the rotation of …

2019 Astronomy and Astrophysics
SOHO 52
An alternative interpretation of the exomoon candidate signal in the combined Kepler and Hubble data of Kepler-1625
DOI: 10.1051/0004-6361/201834913 Bibcode: 2019A&A...624A..95H

Heller, René; Rodenbeck, Kai; Bruno, Giovanni

Context. Kepler and Hubble photometry of a total of four transits by the Jupiter-sized exoplanet Kepler-1625 b have recently been interpreted to show evidence of a Neptune-sized exomoon. The key arguments were an apparent drop in stellar brightness after the planet's October 2017 transit seen with Hubble and its 77.8 min early arrival compared to …

2019 Astronomy and Astrophysics
Gaia eHST 51
VISION - Vienna survey in Orion. III. Young stellar objects in Orion A
DOI: 10.1051/0004-6361/201832577 Bibcode: 2019A&A...622A.149G

Meingast, Stefan; Alves, João; Bouy, Hervé +14 more

We have extended and refined the existing young stellar object (YSO) catalogs for the Orion A molecular cloud, the closest massive star-forming region to Earth. This updated catalog is driven by the large spatial coverage (18.3 deg2, ∼950 pc2), seeing limited resolution (∼0.7″), and sensitivity (Ks < 19 mag) of …

2019 Astronomy and Astrophysics
Herschel 51