Search Publications

Phase reddening on asteroid Bennu from visible and near-infrared spectroscopy
DOI: 10.1051/0004-6361/202039552 Bibcode: 2020A&A...644A.142F

Barucci, M. A.; Fornasier, S.; Li, J. -Y. +10 more

Context. The NASA mission OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) has been observing near-Earth asteroid (101955) Bennu in close proximity since December 2018. In October 2020, the spacecraft collected a sample of surface material from Bennu to return to Earth.
Aims: In this work,…

2020 Astronomy and Astrophysics
Rosetta 29
High-resolution, 3D radiative transfer modelling. III. The DustPedia barred galaxies
DOI: 10.1051/0004-6361/201936176 Bibcode: 2020A&A...637A..25N

Clark, Christopher J. R.; Mosenkov, Aleksandr V.; De Looze, Ilse +17 more

Context. Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating is mainly attributable to the absorption of ultraviolet and optical photons emitted by the youngest (≤100 Myr) stars. Consequently, thermal re-emission by dust at far-i…

2020 Astronomy and Astrophysics
Herschel 29
A multiplicity study of transiting exoplanet host stars. II. Revised properties of transiting planetary systems with companions
DOI: 10.1051/0004-6361/201937334 Bibcode: 2020A&A...635A..74S

Ginski, C.; Southworth, J.; Mancini, L. +2 more

Context. Binarity is a widespread phenomenon around solar-type stars, including the host stars of transiting extrasolar planets.
Aims: We performed a detailed study of six transiting planetary systems with relatively bright stars close enough to affect observations of these systems. These contaminants were characterised in a companion work. <…

2020 Astronomy and Astrophysics
Gaia 29
First detection of ozone in the mid-infrared at Mars: implications for methane detection
DOI: 10.1051/0004-6361/202038125 Bibcode: 2020A&A...639A.141O

Montmessin, F.; Fedorova, A.; Korablev, O. +9 more


Aims: The ExoMars Trace Gas Orbiter was sent to Mars in March 2016 to search for trace gases diagnostic of active geological or biogenic processes.
Methods: We report the first observation of the spectral features of Martian ozone (O3) in the mid-infrared range using the Atmospheric Chemistry Suite Mid-InfaRed (MIR) channel, a…

2020 Astronomy and Astrophysics
ExoMars-16 29
Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies. Insights into dust distributions and star-formation rates at z ∼ 2
DOI: 10.1051/0004-6361/201936286 Bibcode: 2020A&A...635A.119C

Smail, I.; Thomson, A. P.; Dunlop, J. S. +15 more

By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral field spectrographs, including both Spectrograph for INtegral Field Observations in the Near Infrared and K-band Multi Object Spectrograph on the Very Large Telescope, we investigate the two-dimensional distributions of Hα and rest-frame far-infrar…

2020 Astronomy and Astrophysics
Gaia eHST 29
Masses for the seven planets in K2-32 and K2-233. Four diverse planets in resonant chain and the first young rocky worlds
DOI: 10.1051/0004-6361/202037896 Bibcode: 2020A&A...640A..48L

Deleuil, M.; Adibekyan, V.; Sousa, S. G. +18 more

Context. High-precision planetary densities are key pieces of information necessary to derive robust atmospheric properties for extrasolar planets. Measuring precise masses is the most challenging part of this task, especially in multi-planetary systems. The ESO-K2 collaboration focuses on the follow-up of a selection of multi-planetary systems de…

2020 Astronomy and Astrophysics
Gaia 29
Fragmentation of star-forming filaments in the X-shaped nebula of the California molecular cloud
DOI: 10.1051/0004-6361/202037721 Bibcode: 2020A&A...642A..76Z

André, Ph.; Men'shchikov, A.; Wang, Ke +1 more

Context. Dense molecular filaments are central to the star formation process, but the detailed manner in which they fragment into prestellar cores is not well understood yet.
Aims: Here, we investigate the fragmentation properties and dynamical state of several star-forming filaments in the X-shaped nebula region of the California molecular c…

2020 Astronomy and Astrophysics
Gaia Herschel 29
Discovery of new stellar groups in the Orion complex. Towards a robust unsupervised approach
DOI: 10.1051/0004-6361/201935955 Bibcode: 2020A&A...643A.114C

Alves, João; Adamo, Angela; D'Onghia, Elena +1 more

We test the ability of two unsupervised machine learning algorithms, EnLink and Shared Nearest Neighbor (SNN), to identify stellar groupings in the Orion star-forming complex as an application to the 5D astrometric data from Gaia DR2. The algorithms represent two distinct approaches to limiting user bias when selecting parameter values and evaluat…

2020 Astronomy and Astrophysics
Gaia 29
The Fornax 3D project: Globular clusters tracing kinematics and metallicities
DOI: 10.1051/0004-6361/202037685 Bibcode: 2020A&A...637A..26F

Viaene, S.; Hilker, M.; Pinna, F. +15 more

Globular clusters (GCs) are found ubiquitously in massive galaxies and due to their old ages, they are regarded as fossil records of galaxy evolution. Spectroscopic studies of GC systems are often limited to the outskirts of galaxies, where GCs stand out against the galaxy background and serve as bright tracers of galaxy assembly. In this work, we…

2020 Astronomy and Astrophysics
eHST 29
The Gaia-ESO Survey: detection and characterisation of single-line spectroscopic binaries
DOI: 10.1051/0004-6361/201935819 Bibcode: 2020A&A...635A.155M

Gilmore, G.; Bayo, A.; Mowlavi, N. +26 more

Context. Multiple stellar systems play a fundamental role in the formation and evolution of stellar populations in galaxies. Recent and ongoing large ground-based multi-object spectroscopic surveys significantly increase the sample of spectroscopic binaries (SBs) allowing analyses of their statistical properties.
Aims: We investigate the repe…

2020 Astronomy and Astrophysics
Gaia 29