Search Publications

The origin of close massive binaries in the M17 star-forming region
DOI: 10.1051/0004-6361/202141849 Bibcode: 2022A&A...663A..26B

Sana, H.; Frost, A. J.; Reggiani, M. +5 more

Context. Spectroscopic multiplicity surveys of O stars in young clusters and OB associations have revealed that a large portion (∼70%) of these massive stars (Mi > 15 M) belong to close and short-period binaries (with a physical separation of less than a few astronomical units). Follow-up VLT(I) high-angular-resolution ob…

2022 Astronomy and Astrophysics
Gaia 21
FEEDBACK from the NGC 7538 H II region
DOI: 10.1051/0004-6361/202142689 Bibcode: 2022A&A...659A..77B

Schneider, N.; Beuther, H.; Tielens, A. G. G. M. +10 more

Context. The interaction of expanding H II regions with their environmental clouds is one of the central questions driving the Stratospheric Observatory for Infrared Astronomy (SOFIA) legacy program FEEDBACK.
Aims: We want to understand the interaction of the prototypical NGC 7538 H II region with the neighboring molecular cloud hosting sever…

2022 Astronomy and Astrophysics
Herschel 21
Atomic and molecular gas from the epoch of reionisation down to redshift 2
DOI: 10.1051/0004-6361/202142264 Bibcode: 2022A&A...657A..47M

Ciardi, Benedetta; Péroux, Céline; Maio, Umberto

Context. Cosmic gas makes up about 90% of the baryonic matter in the Universe and H2 molecule is the most tightly linked to star formation.
Aims: In this work we study cold neutral gas, its H2 component at different epochs, and corresponding depletion times.
Methods: We perform state-of-the-art hydrodynamic simulati…

2022 Astronomy and Astrophysics
Herschel eHST 21
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline
DOI: 10.1051/0004-6361/202141717 Bibcode: 2022A&A...657A..35G

Sobral, David; Lee, Young Sun; Placco, Vinicius M. +25 more

Context. We explore the stellar content of the Javalambre Photometric Local Universe Survey (J-PLUS) Data Release 2 and show its potential for identifying low-metallicity stars using the Stellar Parameters Estimation based on Ensemble Methods (SPEEM) pipeline.
Aims: SPEEM is a tool used to provide determinations of atmospheric parameters for …

2022 Astronomy and Astrophysics
Gaia 21
Successive deuteration in low-mass star-forming regions: The case of D2-methanol (CHD2OH) in IRAS 16293-2422
DOI: 10.1051/0004-6361/202142863 Bibcode: 2022A&A...659A..69D

Margulès, Laurent; Drozdovskaya, Maria N.; Jørgensen, Jes K. +3 more

Context. Di-deuterated molecules are observed in the earliest stages of star formation at abundances of a few percent relative to their nondeuterated isotopologs, which is unexpected considering the scarcity of deuterium in the interstellar medium. With sensitive observations leading to the detection of a steadily increasing number of di-deuterate…

2022 Astronomy and Astrophysics
Rosetta 21
A scaled-up planetary system around a supernova progenitor
DOI: 10.1051/0004-6361/202243675 Bibcode: 2022A&A...664A...9S

Quanz, S. P.; Henning, T.; Mayer, L. +24 more

Context. Virtually all known exoplanets reside around stars with M < 2.3 M either due to the rapid evaporation of the protostellar disks or to selection effects impeding detections around more massive stellar hosts.
Aims: To clarify if this dearth of planets is real or a selection effect, we launched the planet-hunting B-star E…

2022 Astronomy and Astrophysics
Gaia 21
A CO isotopologue Line Atlas within the Whirlpool galaxy Survey (CLAWS)
DOI: 10.1051/0004-6361/202142247 Bibcode: 2022A&A...662A..89D

Kruijssen, J. M. Diederik; Leroy, Adam K.; Rosolowsky, Erik +24 more

We present the CO isotopologue Line Atlas within the Whirpool galaxy Survey (CLAWS), which is based on an IRAM 30 m large programme that provides a benchmark study of numerous faint CO isotopologues in the millimetre-wavelength regime across the full disc of the nearby grand-design spiral galaxy M 51 (NGC 5194). The survey's core goal is to use th…

2022 Astronomy and Astrophysics
eHST 21
COSMOS2020: UV-selected galaxies at z ≥ 7.5
DOI: 10.1051/0004-6361/202243088 Bibcode: 2022A&A...667A..65K

Sanders, D. B.; Ilbert, O.; Kartaltepe, J. S. +16 more

This paper presents a new search for z ≥ 7.5 galaxies using the COSMOS2020 photometric catalogues. Finding galaxies at the reionisation epoch through deep imaging surveys remains observationally challenging. The larger area covered by ground-based surveys such as COSMOS enables the discovery of the brightest galaxies at these high redshifts. Cover…

2022 Astronomy and Astrophysics
eHST 21
Characteristics and evolution of sheath and leading edge structures of interplanetary coronal mass ejections in the inner heliosphere based on Helios and Parker Solar Probe observations
DOI: 10.1051/0004-6361/202243291 Bibcode: 2022A&A...665A..70T

Temmer, M.; Bothmer, V.

Context. We investigated the plasma and magnetic field characteristics of the upstream regions of interplanetary coronal mass ejections (ICMEs) and their evolution as function of distance to the Sun in the inner heliosphere. Results are related both to the development of interplanetary shocks, sheath regions, and compressed solar wind plasma ahead…

2022 Astronomy and Astrophysics
SOHO 21
Prominence eruption observed in He II 304 Å up to >6 R by EUI/FSI aboard Solar Orbiter
DOI: 10.1051/0004-6361/202244020 Bibcode: 2022A&A...662L...5M

Heinzel, P.; Mierla, M.; Zhukov, A. N. +24 more


Aims: We report observations of a unique, large prominence eruption that was observed in the He II 304 Å passband of the Extreme Ultraviolet Imager/Full Sun Imager telescope aboard Solar Orbiter on 15-16 February 2022.
Methods: Observations from several vantage points - Solar Orbiter, the Solar-Terrestrial Relations Observatory, the Sola…

2022 Astronomy and Astrophysics
SOHO SolarOrbiter 21