Search Publications

The galaxy group merger origin of the Cloverleaf odd radio circle system
DOI: 10.1051/0004-6361/202449900 Bibcode: 2024A&A...685L...2B

Zhang, X.; Nandra, K.; Merloni, A. +14 more

Odd radio circles (ORCs) are a newly discovered class of extended faint radio sources of unknown origin. We report the first detection of diffuse X-ray gas at the location of a low-redshift ORC (z = 0.046) known as Cloverleaf ORC. This observation was performed with the XMM-Newton X-ray telescope. The physical extent of the diffuse X-ray emission …

2024 Astronomy and Astrophysics
XMM-Newton 3
A deep-learning approach to the 3D reconstruction of dust density and temperature in star-forming regions
DOI: 10.1051/0004-6361/202347758 Bibcode: 2024A&A...683A.246K

Klessen, Ralf S.; Testi, Leonardo; Hennebelle, Patrick +8 more


Aims: We introduce a new deep-learning approach for the reconstruction of 3D dust density and temperature distributions from multi-wavelength dust emission observations on the scale of individual star-forming cloud cores (<0.2 pc).
Methods: We constructed a training data set by processing cloud cores from the Cloud Factory simulations…

2024 Astronomy and Astrophysics
Herschel 3
Slitless spectrophotometry with forward modelling: Principles and application to measuring atmospheric transmission
DOI: 10.1051/0004-6361/202347422 Bibcode: 2024A&A...684A..21N

Copin, Y.; Le Guillou, L.; Moniez, M. +9 more

Context. In the next decade, many optical surveys will aim to answer the question of the nature of dark energy by measuring its equation-of-state parameter at the per mill level. This requires trusting the photometric calibration of the survey with a precision never reached so far on many sources of systematic uncertainties. The measurement of the…

2024 Astronomy and Astrophysics
Gaia 3
Revisiting empirical solar energetic particle scaling relations: II. Coronal mass ejections
DOI: 10.1051/0004-6361/202450705 Bibcode: 2024A&A...690A..60P

Veronig, Astrid M.; Papaioannou, Athanasios; Herbst, Konstantin +2 more

Aims. The space radiation environment conditions and the maximum expected coronal mass ejection (CME) speed are assessed by investigating scaling laws between the peak proton flux and fluence of solar energetic particle (SEP) events with the speed of the CMEs. Methods. We used a complete catalog of SEP events, covering the last ∼25 years of CME ob…

2024 Astronomy and Astrophysics
SOHO 3
Stellar model tests and age determination for RGB stars from the APO-K2 catalogue
DOI: 10.1051/0004-6361/202451730 Bibcode: 2024A&A...690A.323V

Valle, G.; Dell'Omodarme, M.; Prada Moroni, P. G. +1 more

Aims. By adopting the recently empirically derived dependence of α-elements on [α/Fe] instead of the conventionally applied uniform one, we tested the agreement between stellar model predictions and observations for red giant branch (RGB) stars in the APO-K2 catalogue. We particularly focused on the biases in effective temperature scales and on th…

2024 Astronomy and Astrophysics
Gaia 3
A long-term study of the magnetic field and activity in the M giant RZ Ari. Magnetism and planet engulfment in a fairly evolved star?
DOI: 10.1051/0004-6361/202346949 Bibcode: 2024A&A...681A..36K

Mathias, P.; Zamanov, R.; Baron, F. +12 more


Aims: We present a detailed long-term study of the single M6 III giant RZ Ari to obtain direct and simultaneous measurements of the magnetic field, activity indicators, and radial velocity in order to infer the origin of its activity. We study its magnetic activity in the context of stellar evolution, and for this purpose, we also refined its…

2024 Astronomy and Astrophysics
Gaia 3
XMM-Newton - NuSTAR monitoring campaign of the Seyfert 1 galaxy IC 4329A
DOI: 10.1051/0004-6361/202348760 Bibcode: 2024A&A...687A..51T

Paltani, S.; Tombesi, F.; Privon, G. C. +13 more

We present the results of a joint XMM-Newton and NuSTAR campaign on the active galactic nucleus (AGN) IC 4329A, consisting of 9 × 20 ks XMM-Newton observations, and 5 × 20 ks NuSTAR observations within nine days, performed in August 2021. Within each observation, the AGN is not very variable, and the fractional variability never exceeds 5%. Flux v…

2024 Astronomy and Astrophysics
Exosat XMM-Newton 3
Eight new 2+2 doubly eclipsing quadruple systems detected
DOI: 10.1051/0004-6361/202450400 Bibcode: 2024A&A...687A...6Z

Merc, J.; Kučáková, H.; Zasche, P. +2 more

We studied eight new doubly eclipsing stellar systems. We found that they are all rare examples of quadruple systems of 2 + 2 architecture, where both inner pairs are eclipsing binaries. Until now, such a configuration had only been proven for dozens of systems on the whole sky. We enlarged this rare group of systems with four stars in the Small M…

2024 Astronomy and Astrophysics
Gaia 3
The Smallest Scale of Hierarchy Survey (SSH): III. Dwarf-dwarf satellite merging phenomena in the low-mass regime
DOI: 10.1051/0004-6361/202450106 Bibcode: 2024A&A...691A..65S

de Jong, Roelof S.; Cannon, John M.; Cignoni, Michele +13 more

We present new deep, wide-field imaging data from the Large Binocular Telescope (LBT) in g and r bands from the Smallest Scale of Hierarchy Survey (SSH) that reveal previously undetected tidal features and stellar streams in the outskirts of six dwarf irregular galaxies (NGC 5238, UGC 6456, UGC 6541, UGC 7605, UGC 8638, and UGC 8760) with stellar …

2024 Astronomy and Astrophysics
eHST 3
Dust mass in protoplanetary disks with porous dust opacities
DOI: 10.1051/0004-6361/202451981 Bibcode: 2024A&A...692A.148L

Fang, Min; Flock, Mario; Henning, Thomas +8 more

Atacama Large Millimeter/submillimeter Array surveys have suggested that protoplanetary disks are not massive enough to form the known exoplanet population, based on the assumption that the millimeter continuum emission is optically thin. In this work, we investigate how the mass determination is influenced when the porosity of dust grains is cons…

2024 Astronomy and Astrophysics
Herschel 3