Search Publications

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
Detection and characterisation of 54 massive companions with the SOPHIE spectrograph. Seven new brown dwarfs and constraints on the brown dwarf desert
DOI: 10.1051/0004-6361/201935113 Bibcode: 2019A&A...631A.125K

Bouchy, F.; Deleuil, M.; Moutou, C. +35 more

Context. Brown dwarfs (BD) are substellar objects intermediate between planets and stars with masses of ~13-80 MJ. While isolated BDs are most likely produced by gravitational collapse in molecular clouds down to masses of a few MJ, a non-negligible fraction of low-mass companions might be formed through the planet-formation …

2019 Astronomy and Astrophysics
Gaia Hipparcos 51
Gaia DR 2 and VLT/FLAMES search for new satellites of the LMC
DOI: 10.1051/0004-6361/201833458 Bibcode: 2019A&A...623A.129F

Carrera, R.; Fritz, T. K.; Battaglia, G. +1 more

A wealth of tiny galactic systems populates the surroundings of the Milky Way. However, some of these objects might have originated as former satellites of the Magellanic Clouds, in particular of the Large Magellanic Cloud (LMC). Examples of the importance of understanding how many systems are genuine satellites of the Milky Way or the LMC are the…

2019 Astronomy and Astrophysics
Gaia 51
New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
DOI: 10.1051/0004-6361/201935597 Bibcode: 2019A&A...631A..87V

Inami, H.; Steinmetz, M.; Richard, J. +8 more

It remains a challenge to assess the merger fraction of galaxies at different cosmic epochs in order to probe the evolution of their mass assembly. Using the ILLUSTRIS cosmological simulation project, we investigate the relation between the separation of galaxies in a pair, both in velocity and projected spatial separation space, and the probabili…

2019 Astronomy and Astrophysics
eHST 51
Catalog for the ESPRESSO blind radial velocity exoplanet survey
DOI: 10.1051/0004-6361/201834729 Bibcode: 2019A&A...629A..80H

Rebolo, R.; Zapatero Osorio, M. R.; Poretti, E. +19 more


Aims: One of the main scientific drivers for ESPRESSO, Échelle SPectrograph, is the detection and characterization of Earth-class exoplanets. With this goal in mind, the ESPRESSO guaranteed time observations (GTO) Catalog identifies the best target stars for a blind search for the radial velocity (RV) signals caused by Earth-class exoplanets.…

2019 Astronomy and Astrophysics
Gaia 51