Search Publications

The XXL Survey. XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z ∼ 1: a multi-wavelength approach
DOI: 10.1051/0004-6361/201937249 Bibcode: 2020A&A...642A.126R

Chiappetti, L.; Berta, S.; Altieri, B. +61 more

High-mass clusters at low redshifts have been intensively studied at various wavelengths. However, while more distant objects at lower masses constitute the bulk population of future surveys, their physical state remain poorly explored to date. In this paper, we present resolved observations of the Sunyaev-Zel'dovich (SZ) effect, obtained with the…

2020 Astronomy and Astrophysics
XMM-Newton 10
Multi-wavelength campaign on NGC 7469. V. Analysis of the HST/COS observations: Super solar metallicity, distance, and trough variation models
DOI: 10.1051/0004-6361/201935342 Bibcode: 2020A&A...633A..61A

Kaastra, J. S.; Kriss, G. A.; Arav, N. +18 more

Context. AGN outflows are thought to influence the evolution of their host galaxies and their super massive black holes. To better understand these outflows, we executed a deep multiwavelength campaign on NGC 7469. The resulting data, combined with those of earlier epochs, allowed us to construct a comprehensive physical, spatial, and temporal pic…

2020 Astronomy and Astrophysics
eHST 10
CS Cha B: A disc-obscured M-type star mimicking a polarised planetary companion
DOI: 10.1051/0004-6361/202038706 Bibcode: 2020A&A...640L..12H

Snellen, I. A. G.; Ginski, C.; Girard, J. +6 more

Context. Direct imaging provides a steady flow of newly discovered giant planets and brown dwarf companions. These multi-object systems can provide information about the formation of low-mass companions in wide orbits and/or help us to speculate about possible migration scenarios. Accurate classification of companions is crucial for testing format…

2020 Astronomy and Astrophysics
Gaia 10
APEX observations of ortho-H2D+ towards dense cores in the Orion B9 filament
DOI: 10.1051/0004-6361/201936730 Bibcode: 2020A&A...634A.115M

Miettinen, O.

Context. Initial conditions and very early stages of star formation can be probed through spectroscopic observations of deuterated molecular species
Aims: We aim to determine the ortho-H2D+ properties (e.g. column density and fractional abundance with respect to H2) in a sample of dense cores in the Orion B9 s…

2020 Astronomy and Astrophysics
Herschel 10
Gaia18aen: First symbiotic star discovered by Gaia
DOI: 10.1051/0004-6361/202039132 Bibcode: 2020A&A...644A..49M

Reichart, D. E.; Skowron, J.; Gromadzki, M. +20 more

Context. Besides the astrometric mission of the Gaia satellite, its repeated and high-precision measurements also serve as an all-sky photometric transient survey. The sudden brightenings of the sources are published as Gaia Photometric Science Alerts and are made publicly available, allowing the community to photometrically and spectroscopically …

2020 Astronomy and Astrophysics
Gaia 10
VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201936361 Bibcode: 2020A&A...636A..54V

Kaper, L.; Sabbi, E.; de Mink, S. E. +13 more

The process of massive star (M ≥ 8 M) formation is still poorly understood. Observations of massive young stellar objects (MYSOs) are challenging due to their rarity, short formation timescale, large distances, and high circumstellar extinction. Here, we present the results of a spectroscopic analysis of a population of MYSOs in the La…

2020 Astronomy and Astrophysics
Gaia 10
Cold gas and dust: Hunting spiral-like structures in early-type galaxies
DOI: 10.1051/0004-6361/201935090 Bibcode: 2020A&A...636A...8Y

Duc, P. -A.; Peletier, R. F.; Serra, P. +1 more

Context. Observations of neutral hydrogen (H I) and molecular gas show that 50% of all nearby early-type galaxies contain some cold gas. Molecular gas is always found in small gas discs in the central region of the galaxy, while neutral hydrogen is often distributed in a low-column density disc or ring typically extending well beyond the stellar b…

2020 Astronomy and Astrophysics
Herschel 10
FEDReD. I. 3D extinction and stellar maps by Bayesian deconvolution
DOI: 10.1051/0004-6361/202037466 Bibcode: 2020A&A...641A..78B

Arenou, F.; Babusiaux, C.; Hottier, C. +2 more

Context. While Gaia enables us to probe the extended local neighbourhood in great detail, the thin disc structure at larger distances remains sparsely explored.
Aims: We aim here to build a non-parametric 3D model of the thin disc structures handling both the extinction and the stellar density simultaneously.
Methods: We developed a Baye…

2020 Astronomy and Astrophysics
Gaia 10
Impact of a companion and of chromospheric emission on the shape of chromosome maps for globular clusters
DOI: 10.1051/0004-6361/201937212 Bibcode: 2020A&A...635A..52M

Martins, F.; Lardo, C.; Morin, J. +2 more

Context. Globular clusters (GCs) host multiple populations of stars that are well-separated in a photometric diagram - the chromosome map - built from specific Hubble Space Telescope (HST) filters. Stars from different populations feature at various locations on this diagram due to peculiar chemical compositions. Stars of the first population, wit…

2020 Astronomy and Astrophysics
eHST 10
The GAPS programme at TNG. XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone
DOI: 10.1051/0004-6361/202037954 Bibcode: 2020A&A...641A..68B

Scandariato, G.; Pagano, I.; Poretti, E. +34 more

Context. With the growth of comparative exoplanetology, it is becoming increasingly clear that investigating the relationships between inner and outer planets plays a key role in discriminating between competing formation and evolution models. To do so, it is important to probe the inner region of systems that host long-period giants in search of …

2020 Astronomy and Astrophysics
Gaia 10