Search Publications

The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies
DOI: 10.1051/0004-6361/202451006 Bibcode: 2024A&A...691A.299G

Smail, Ian; Brammer, Gabe; Swinbank, A. M. +15 more

We present an analysis of the JWST NIRCam and MIRI morphological and structural properties of 80 massive (log10(M*[M]) = 11.2 ± 0.1) dusty star-forming galaxies at z = 2.7‑0.7+1.2, identified as sub-millimetre galaxies (SMGs) by ALMA, which have been observed as part of the JWST PRIMER projec…

2024 Astronomy and Astrophysics
Gaia eHST JWST 18
Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal). I. The formation and evolution of the thin disc from the Gaia Catalogue of Nearby Stars
DOI: 10.1051/0004-6361/202349078 Bibcode: 2024A&A...687A.168G

Ruiz-Lara, Tomás; Vasiliev, Eugene; Chiappini, Cristina +15 more

Context. The study of the Milky Way is living a golden era thanks to the enormous high-quality datasets delivered by Gaia, and space asteroseismic and ground-based spectroscopic surveys. However, the current major challenge to reconstructing the chronology of the Milky Way is the difficulty to derive precise stellar ages for large samples of stars…

2024 Astronomy and Astrophysics
Gaia 18
MINDS: The DR Tau disk. I. Combining JWST-MIRI data with high-resolution CO spectra to characterise the hot gas
DOI: 10.1051/0004-6361/202348911 Bibcode: 2024A&A...686A.117T

Henning, Thomas; Waters, L. B. F. M.; Güdel, Manuel +29 more

Context. The MRS mode of the JWST-MIRI instrument has been shown to be a powerful tool to characterise the molecular gas emission of the inner region of planet-forming disks. Investigating their spectra allows us to infer the composition of the gas in these regions and, subsequently, the potential atmospheric composition of the forming planets. We…

2024 Astronomy and Astrophysics
JWST 18
Fast-rotating massive Population III stars as possible sources of extreme N enrichment in high-redshift galaxies
DOI: 10.1051/0004-6361/202348866 Bibcode: 2024A&A...688A.142N

Sibony, Yves; Nandal, Devesh; Tsiatsiou, Sophie

We present an analysis of the chemical compositions in high-redshift galaxies, with a focus on the nitrogen-enhanced galaxies GN-z11 and CEERS-1019. We used stellar models of massive stars with initial masses ranging from 9 to 120 M and various metallicities to deduce the chemical abundances of stellar ejecta for a few light elements (…

2024 Astronomy and Astrophysics
JWST 18
JWST observations of 13CO2 ice. Tracing the chemical environment and thermal history of ices in protostellar envelopes
DOI: 10.1051/0004-6361/202348718 Bibcode: 2024A&A...685A..27B

Manoj, P.; Narang, Mayank; Bourke, Tyler L. +38 more

The structure and composition of simple ices can be severely modified during stellar evolution by protostellar heating. Key to understanding the involved processes are thermal and chemical tracers that can be used to diagnose the history and environment of the ice. The 15.2 µm bending mode of 12CO2 in particular has proven to…

2024 Astronomy and Astrophysics
JWST 18
The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ∼ 2
DOI: 10.1051/0004-6361/202348095 Bibcode: 2024A&A...687A..61M

Sanders, D. B.; Ilbert, O.; Kartaltepe, J. S. +35 more


Aims: We provide an in-depth analysis of the COSMOS-Web ring, an Einstein ring at z ≈ 2 that we serendipitously discovered during the data reduction of the COSMOS-Web survey and that could be the most distant lens discovered to date.
Methods: We extracted the visible and near-infrared photometry of the source and the lens from more than …

2024 Astronomy and Astrophysics
Herschel eHST JWST 18
IXPE observation confirms a high spin in the accreting black hole 4U 1957+115
DOI: 10.1051/0004-6361/202348277 Bibcode: 2024A&A...684A..95M

Antonelli, L. A.; Costa, E.; Bianchi, S. +113 more

We present the results of the first X-ray polarimetric observation of the low-mass X-ray binary 4U 1957+115, performed with the Imaging X-ray Polarimetry Explorer in May 2023. The binary system has been in a high-soft spectral state since its discovery and is thought to host a black hole. The ∼571 ks observation reveals a linear polarisation degre…

2024 Astronomy and Astrophysics
Gaia 17
X-Shooting ULLYSES: Massive stars at low metallicity: VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
DOI: 10.1051/0004-6361/202449665 Bibcode: 2024A&A...692A..90R

Wang, L.; Hamann, W. -R.; Oey, M. S. +16 more

On the route toward merging neutron stars and stripped-envelope supernovae, binary population synthesis predicts a large number of post-interaction systems with massive stars that have been stripped of their outer layers. However, observations of such stars in the intermediate-mass regime below the Wolf-Rayet masses are rare. Using X-Shooting ULLY…

2024 Astronomy and Astrophysics
eHST 17
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+1
DOI: 10.1051/0004-6361/202449318 Bibcode: 2024A&A...688A.170B

Done, Chris; Kaaret, Philip; Wu, Kinwah +106 more

Weakly magnetized neutron stars in X-ray binaries show a complex phenomenology with several spectral components that can be associated with the accretion disk, the boundary, and/or a spreading layer, a corona, and a wind. Spectroscopic information alone, however, is not enough to distinguish these components. The analysis of the timing data reveal…

2024 Astronomy and Astrophysics
XMM-Newton 17
2D disc modelling of the JWST line spectrum of EX Lupi
DOI: 10.1051/0004-6361/202347730 Bibcode: 2024A&A...683A.219W

Woitke, P.; Kamp, I.; Ábrahám, P. +3 more

We introduce a number of improvements to the thermo-chemical disc modelling code PRODIMO and new theoretical approaches that can be used to better predict and analyse the JWST line spectra of protoplanetary discs. We developed a new line escape probability method for disc geometries, and a new scheme for dust settling, and discuss how to apply UV …

2024 Astronomy and Astrophysics
Herschel XMM-Newton 17