Search Publications

Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues. I. Methodology and first application in the COSMOS field
DOI: 10.1051/0004-6361/202349055 Bibcode: 2024A&A...688A..20W

Jarvis, Matt J.; Pearson, William J.; Vaccari, Mattia +12 more

Context. Single-dish far-infrared (far-IR) and sub-millimetre (sub-mm) point source catalogues and their connections with galaxy catalogues at other wavelengths are of paramount importance to studying galaxy evolution. However, due to the large mismatch in spatial resolution, cross-matching galaxies detected at different wavelengths is not straigh…

2024 Astronomy and Astrophysics
Herschel 1
High-resolution imaging of the evolving bipolar outflows in symbiotic novae: The case of the RS Ophiuchi 2021 nova outburst
DOI: 10.1051/0004-6361/202451364 Bibcode: 2024A&A...692A.107L

Munari, U.; Giroletti, M.; Williams, D. R. A. +6 more

Context. The recurrent and symbiotic nova RS Ophiuchi (RS Oph) underwent a new outburst phase during August 2021, about 15 years after the last event that occurred in 2006. This outburst represents the first nova event ever detected at very high energies (VHE, E > 100 GeV), and a whole set of coordinated multiwavelength observations were trigge…

2024 Astronomy and Astrophysics
Gaia 1
Confirmation of the presence of a CRSF in the NICER spectrum of X 1822-371
DOI: 10.1051/0004-6361/202345888 Bibcode: 2024A&A...683A..79I

Sanna, A.; Di Salvo, T.; Burderi, L. +6 more


Aims: X 1822-371 is an eclipsing binary system with a period close to 5.57 h and an orbital period derivative Ṗorb of 1.42(3) × 10−10 s s−1. The extremely high value of its Ṗorb is compatible with a super-Eddington mass transfer rate from the companion star and, consequently, an intrinsic luminosity…

2024 Astronomy and Astrophysics
XMM-Newton 1
Coronal and chromospheric activity of Teegarden's star
DOI: 10.1051/0004-6361/202451697 Bibcode: 2024A&A...691A.208F

Schmitt, J. H. M. M.; Czesla, S.; Reiners, A. +11 more

Teegarden's star is a late-type M-dwarf planet host, typically showing only rather low levels of activity. In this paper we present an extensive characterisation of this activity at photospheric, chromospheric, and coronal levels. We specifically investigated TESS observations of Teegarden's star, which showed two very large flares with an estimat…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 1
Extreme magnetic field modulus variability of the Bp star HD 57372
DOI: 10.1051/0004-6361/202449630 Bibcode: 2024A&A...687A.282H

Ilyin, I.; Hubrig, S.; Järvinen, S. P. +2 more

Context. In chemically peculiar Ap/Bp stars with large-scale organised magnetic fields of simple centred dipole configuration, the ratio between the maximum and the minimum of the mean magnetic field modulus is on the order of 1.25. Values of two or more are observed only for very few Ap/Bp stars and are indicative of a very unusual magnetic field…

2024 Astronomy and Astrophysics
Gaia 1
The disk of the eruptive protostar V900 Mon. A MATISSE/VLTI and MUSE/VLT perspective
DOI: 10.1051/0004-6361/202245740 Bibcode: 2024A&A...682A..75L

Lykou, F.; Ábrahám, P.; Chen, L. +8 more


Aims: In this work, we study the silicate dust content in the disk of one of the youngest eruptive stars, V900 Mon, at the highest angular resolution, probing down to the inner 10 au of said disk, and study the historical evolution of the system, traced in part by a newly discovered emission clump.
Methods: We performed high angular reso…

2024 Astronomy and Astrophysics
AKARI Gaia 1
Dynamical traceback age of the Octans young stellar association
DOI: 10.1051/0004-6361/202449549 Bibcode: 2024A&A...689A..11G

Miret-Roig, N.; Bouy, H.; Barrado, D. +2 more

Context. Octans is one of the most distant (d ∼ 150 pc) young stellar associations of the solar neighbourhood, and it has not yet been sufficiently explored. Its age is still poorly constrained in the literature and requires further investigation.
Aims: We take advantage of the state-of-the-art astrometry delivered by the third data release o…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 1
The debiased morphological transformations of galaxies since z = 3 in CANDELS
DOI: 10.1051/0004-6361/202347522 Bibcode: 2024A&A...684A.166S

Demarco, R.; Cerulo, P.; Salvador, D. +3 more

Context. Morphological quantitative measurements and visual-like classifications are susceptible to biases arising from the expansion of the Universe. One of these biases is the effect of cosmological surface brightness dimming (CSBD): the measured surface brightness of a galaxy decays with redshift as (1 + z)−4. This effect might lead …

2024 Astronomy and Astrophysics
eHST 1
Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720 b, TOI-6008 b, and TOI-6086 b
DOI: 10.1051/0004-6361/202349127 Bibcode: 2024A&A...687A.264B

Tamura, M.; Pallé, E.; Hirano, T. +53 more

One of the main goals of the NASA Transiting Exoplanet Survey Satellite (TESS) mission is the discovery of Earth-like planets around nearby M-dwarf stars. We present the discovery and validation of three new short-period Earth-sized planets orbiting nearby M dwarfs: TOI-5720 b, TOI-6008 b, and TOI-6086 b. We combined TESS data, ground-based multic…

2024 Astronomy and Astrophysics
Gaia 1
First detection of CF+ in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/202449429 Bibcode: 2024A&A...687A..29G

Gong, Yan; Menten, Karl M.; Jacob, Arshia M. +2 more

Context. CF+ has been established as a valuable diagnostic tool for investigating photodissociation regions (PDRs) and fluorine abundances in the Milky Way. However, its role in extragalactic environments remains largely uncharted.
Aims: Our objective is to explore the significance of CF+ in the Large Magellanic Cloud (L…

2024 Astronomy and Astrophysics
Herschel 1