Search Publications

MINCE. II. Neutron capture elements
DOI: 10.1051/0004-6361/202449539 Bibcode: 2024A&A...686A.295F

Steffen, M.; Hansen, C. J.; Bonifacio, P. +24 more

Context. Most of the studies on the determination of the chemical composition of metal-poor stars have been focused on the search of the most pristine stars, searching for the imprints of the ejecta of the first supernovae. Apart from the rare and very interesting r-enriched stars, few elements are measurable in the very metal-poor stars. On the o…

2024 Astronomy and Astrophysics
Gaia 10
Age uncertainties of red giants due to cumulative rotational mixing of progenitors calibrated by asteroseismology
DOI: 10.1051/0004-6361/202449300 Bibcode: 2024A&A...684A.112F

Aerts, C.; Van Reeth, T.; Fritzewski, D. J. +2 more

Context. Galactic archaeology largely relies on precise ages of distant evolved stars in the Milky Way. Nowadays, asteroseismology can deliver ages for many red giants observed with high-cadence, high-precision photometric space missions such as CoRoT, Kepler, K2, TESS, and soon PLATO.
Aims: Our aim is to quantify the age uncertainties of cur…

2024 Astronomy and Astrophysics
Gaia 10
Variable stars in galactic globular clusters. I. The population of RR Lyrae stars
DOI: 10.1051/0004-6361/202348961 Bibcode: 2024A&A...684A.173C

Anderson, Richard I.; Cruz Reyes, Mauricio; Netzel, Henryka +2 more

We present a comprehensive catalog of 2824 RR Lyrae stars (RRLs) residing in 115 Galactic globular clusters (GCs). Our catalog includes 1594 fundamental-mode (RRab), 824 first-overtone (RRc), and 28 double-mode (RRd) RRLs, as well as 378 RRLs of an unknown pulsation mode. We cross-matched 481 349 RRLs reported in the third Data Release (DR3) of th…

2024 Astronomy and Astrophysics
Gaia 10
Age-dating the young open cluster UBC 1 with g-mode asteroseismology, gyrochronology, and isochrone fitting
DOI: 10.1051/0004-6361/202347618 Bibcode: 2024A&A...681A..13F

Aerts, C.; Li, G.; Van Reeth, T. +3 more


Aims: UBC 1 is an open cluster discovered in Gaia data and located near the edge of the Transiting Exoplanet Survey Satellite's (TESS) continuous viewing zone. We aim to provide age constraints for this poorly studied open cluster from the combination of gravity-mode (g-mode) asteroseismology, gyrochronology, and isochrone fitting.
Metho…

2024 Astronomy and Astrophysics
Gaia 10
Linking Mg II and [O II] spatial distribution to ionizing photon escape in confirmed LyC leakers and non-leakers
DOI: 10.1051/0004-6361/202449362 Bibcode: 2024A&A...687A..73L

Blaizot, Jérémy; Verhamme, Anne; Scarlata, Claudia +29 more

The geometry of the neutral gas in and around galaxies is a key regulator of the escape of ionizing photons. We present the first statistical study aimed at linking the neutral and ionized gas distributions to the Lyman continuum (LyC) escape fraction (fescLyC) in a sample of 22 confirmed LyC leakers and non-leakers at z ≈ 0.…

2024 Astronomy and Astrophysics
eHST 10
Uniting Gaia and APOGEE to unveil the cosmic chemistry of the Milky Way disc
DOI: 10.1051/0004-6361/202348018 Bibcode: 2024A&A...683A.128C

Casey, Andrew R.; Rix, Hans-Walter; Brown, Anthony G. A. +6 more

The spatial distribution of Galactic stars with different chemical abundances encodes information on the processes that drove the formation and evolution of the Milky Way. Survey selection functions are indispensable for analysing astronomical catalogues produced by large-scale surveys. The use of these selection functions in data modelling is mor…

2024 Astronomy and Astrophysics
Gaia 10
Dust mineralogy and variability of the inner PDS 70 disk: Insights from JWST/MIRI MRS and Spitzer IRS observations
DOI: 10.1051/0004-6361/202451589 Bibcode: 2024A&A...691A.148J

Henning, Thomas; Güdel, Manuel; Lagage, Pierre-Olivier +17 more

Context. The inner disk of the young star PDS 70 may be a site of rocky planet formation, with two giant planets detected further out. Recently, James Webb Space Telescope/Mid-Infrared Instrument (JWST/MIRI) Medium-Resolution Spectrometer (MRS) observations have revealed the presence of warm water vapour in the inner disk. Solids in the inner disk…

2024 Astronomy and Astrophysics
JWST 10
LOFAR detection of extended emission around a mini halo in the galaxy cluster Abell 1413
DOI: 10.1051/0004-6361/202347635 Bibcode: 2024A&A...683A.132L

Rossetti, M.; Shimwell, T. W.; Gastaldello, F. +14 more

Context. The relation between giant radio halos and mini halos in galaxy clusters is not understood. The former are usually associated with merging clusters, while the latter are found in relaxed systems. In recent years, the advent of low-frequency radio observations has challenged this dichotomy by finding intermediate objects with a hybrid radi…

2024 Astronomy and Astrophysics
XMM-Newton 10
No evidence of active galactic nucleus features in the nuclei of Arp 220 from JWST/NIRSpec IFS
DOI: 10.1051/0004-6361/202450094 Bibcode: 2024A&A...690A.171P

Charlot, Stéphane; Übler, Hannah; D'Eugenio, Francesco +12 more

Context. Arp 220 is the nearest ultra-luminous infrared galaxy. It shows evidence of 100 pc scale molecular outflows that are likely connected with galaxy-scale outflows traced by ionised and neutral gas. The two highly obscured nuclei of Arp 220 are sites of intense star formation, with extreme (far-infrared based) star formation rate surface den…

2024 Astronomy and Astrophysics
JWST 10
Radial evolution of the accuracy of ballistic solar wind backmapping
DOI: 10.1051/0004-6361/202348892 Bibcode: 2024A&A...686A..12D

Maksimovic, M.; Démoulin, P.; Badman, S. T. +4 more

Context. Solar wind backmapping is a technique employed to connect in situ measurements of heliospheric plasma structures to their origin near the Sun. The most widely used method is ballistic mapping, which neglects the effects of solar wind acceleration and corotation and instead models the solar wind as a constant radial outflow whose speed is …

2024 Astronomy and Astrophysics
Ulysses 10