Search Publications

Luminous red novae: Stellar mergers or giant eruptions?
DOI: 10.1051/0004-6361/201935999 Bibcode: 2019A&A...630A..75P

Drake, A. J.; Sollerman, J.; Djorgovski, S. G. +36 more

We present extensive datasets for a class of intermediate-luminosity optical transients known as luminous red novae. They show double-peaked light curves, with an initial rapid luminosity rise to a blue peak (at -13 to -15 mag), which is followed by a longer-duration red peak that sometimes is attenuated, resembling a plateau. The progenitors of t…

2019 Astronomy and Astrophysics
Gaia 100
Transient processing and analysis using AMPEL: alert management, photometry, and evaluation of light curves
DOI: 10.1051/0004-6361/201935634 Bibcode: 2019A&A...631A.147N

Sollerman, J.; Gal-Yam, A.; Kowalski, M. +18 more

Context. Both multi-messenger astronomy and new high-throughput wide-field surveys require flexible tools for the selection and analysis of astrophysical transients.
Aims: Here we introduce the alert management, photometry, and evaluation of light curves (AMPEL) system, an analysis framework designed for high-throughput surveys and suited for…

2019 Astronomy and Astrophysics
Gaia 99
Towards emulating cosmic shear data: revisiting the calibration of the shear measurements for the Kilo-Degree Survey
DOI: 10.1051/0004-6361/201834819 Bibcode: 2019A&A...624A..92K

Hoekstra, Henk; Heymans, Catherine; Kuijken, Konrad +9 more

Exploiting the full statistical power of future cosmic shear surveys will necessitate improvements to the accuracy with which the gravitational lensing signal is measured. We present a framework for calibrating shear with image simulations that demonstrates the importance of including realistic correlations between galaxy morphology, size, and mor…

2019 Astronomy and Astrophysics
eHST 98
Observation-based modelling of magnetised coronal mass ejections with EUHFORIA
DOI: 10.1051/0004-6361/201935053 Bibcode: 2019A&A...626A.122S

Mierla, M.; Rodriguez, L.; Poedts, S. +2 more

Context. Coronal mass ejections (CMEs) are the primary source of strong space weather disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic pressure and internal magnetic fields, for which reliable predictions at Earth are not possible with traditional cone CME models.
Aims: We study two well-observed Earth-dir…

2019 Astronomy and Astrophysics
SOHO 95
Extended stellar systems in the solar neighborhood. I. The tidal tails of the Hyades
DOI: 10.1051/0004-6361/201834622 Bibcode: 2019A&A...621L...3M

Meingast, Stefan; Alves, João

We report the discovery of two well-defined tidal tails emerging from the Hyades star cluster. The tails were detected in Gaia DR2 data by selecting cluster members in the 3D galactocentric cylindrical velocity space. The robustness of our member selection is reinforced by the fact that the sources depict an almost noiseless, coeval stellar main s…

2019 Astronomy and Astrophysics
Gaia 94
Signatures of the resonances of a large Galactic bar in local velocity space
DOI: 10.1051/0004-6361/201834820 Bibcode: 2019A&A...626A..41M

Monari, G.; Siebert, A.; Famaey, B. +2 more

The second data release of the Gaia mission has revealed a very rich structure in local velocity space. In terms of in-plane motions, this rich structure is also seen as multiple ridges in the actions of the axisymmetric background potential of the Galaxy. These ridges are probably related to a combination of effects from ongoing phase-mixing and …

2019 Astronomy and Astrophysics
Gaia 93
The Herschel Dwarf Galaxy Survey. II. Physical conditions, origin of [C II] emission, and porosity of the multiphase low-metallicity ISM
DOI: 10.1051/0004-6361/201834457 Bibcode: 2019A&A...626A..23C

Lebouteiller, V.; Madden, S. C.; Galliano, F. +7 more

The sensitive infrared telescopes, Spitzer and Herschel, have been used to target low-metallicity star-forming galaxies, allowing us to investigate the properties of their interstellar medium (ISM) in unprecedented detail. Interpretation of the observations in physical terms relies on careful modeling of those properties. We have employed a multip…

2019 Astronomy and Astrophysics
Herschel 93
The ultra-diffuse galaxy NGC 1052-DF2 with MUSE. I. Kinematics of the stellar body
DOI: 10.1051/0004-6361/201834909 Bibcode: 2019A&A...625A..76E

Emsellem, Eric; Müller, Oliver; Lelli, Federico +14 more

The so-called ultra-diffuse galaxy NGC 1052-DF2 was announced to be a galaxy lacking dark matter based on a spectroscopic study of its constituent globular clusters. Here we present the first spectroscopic analysis of the stellar body of this galaxy using the MUSE integral-field spectrograph at the (ESO) Very Large Telescope. The MUSE datacube sim…

2019 Astronomy and Astrophysics
eHST 93
Observational constraints on dust disk sizes in tidally truncated protoplanetary disks in multiple systems in the Taurus region
DOI: 10.1051/0004-6361/201935964 Bibcode: 2019A&A...628A..95M

Liu, Y.; Lodato, G.; van der Plas, G. +16 more

The impact of stellar multiplicity on the evolution of planet-forming disks is still the subject of debate. Here we present and analyze disk structures around ten multiple stellar systems that were included in an unbiased, high spatial resolution survey performed with ALMA of 32 protoplanetary disks in the Taurus star-forming region. At the unprec…

2019 Astronomy and Astrophysics
Gaia 92
Dynamics of cluster-forming hub-filament systems. The case of the high-mass star-forming complex Monoceros R2
DOI: 10.1051/0004-6361/201935260 Bibcode: 2019A&A...629A..81T

Schneider, N.; Tremblin, P.; Didelon, P. +15 more

Context. High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2 (hereafter Mon R2), at a distance of 830 pc, harbors one of the closest of these systems, making it an excellent target for case studies.
Aims: We investigate the morphology, stability and dynamical properties of the Mon R2 hub-filament system. …

2019 Astronomy and Astrophysics
Herschel 91