Search Publications

Spectral similarities in galaxies through an unsupervised classification of spaxels
DOI: 10.1051/0004-6361/202449516 Bibcode: 2024A&A...688A..19C

Fraix-Burnet, D.; Chambon, H. J.


Aims: We present the first unsupervised classification of spaxels in hyperspectral images of individual galaxies. Classes identify regions by spectral similarity and thus take all the information into account that is contained in the data cubes (spatial and spectral).
Methods: We used Gaussian mixture models in a latent discriminant subs…

2024 Astronomy and Astrophysics
JWST 1
Optical polarimetry study of the Lambda-Orionis star-forming region
DOI: 10.1051/0004-6361/202449720 Bibcode: 2024A&A...689A.225N

Neha, S.; Soam, A.; Maheswar, G.

We present an optical polarimetry study of the nearby star-forming region Lambda-Orionis to map the plane-of-the-sky magnetic field geometry to understand the magnetized evolution of the HII region and the associated small molecular clouds. We made multiwavelength polarization observations of 34 bright stars distributed across the region. We also …

2024 Astronomy and Astrophysics
Gaia 1
Multiwavelength observation of 1A 0535+262=HD 245770 from 2010 to 2021
DOI: 10.1051/0004-6361/202347622 Bibcode: 2024A&A...681A..10L

Liu, Wei; Yan, Jingzhi; Xiao, Guangcheng +3 more

Context. 1A 0535+262 is a high-mass X-ray binary that went into a giant X-ray outburst in 2020. During this event, the X-ray luminosity reached the highest value measured over the last 30 years.
Aims: Our aim is to study the long-term variability of 1A 0535+262 before and after the 2020 major X-ray outburst and to uncover the mechanism that l…

2024 Astronomy and Astrophysics
INTEGRAL 1
Characterisation of the X-ray point source variability in the eROSITA south ecliptic pole field
DOI: 10.1051/0004-6361/202449415 Bibcode: 2024A&A...687A..37B

Salvato, M.; Buchner, J.; Nandra, K. +11 more


Aims: During the Spectrum Roentgen Gamma (SRG)/eROSITA all-sky surveys, X-ray sources close to the South Ecliptic Pole (SEP) are observed almost every 4 h. We aim to identify the sources exhibiting the most significant long-term X-ray variability within 3° of the SEP in the first three surveys, and investigate their properties.
Methods: …

2024 Astronomy and Astrophysics
Gaia 1
The true nature of HE 0057-5959, the most metal-poor, Li-rich star
DOI: 10.1051/0004-6361/202449290 Bibcode: 2024A&A...689A..89M

Salaris, M.; Bonifacio, P.; Monaco, L. +2 more

The Li-rich stars are a class of rare objects with a surface lithium abundance, A(Li), that exceeds that of other stars in the same evolutionary stage. The origin of these stars is still debated, and valuable routes to look at include the Cameron-Fowler mechanism, a mass-transfer process in a binary system, or the engulfment of rocky planets or br…

2024 Astronomy and Astrophysics
Gaia 1
Radial velocity homogeneous analysis of M dwarfs observed with HARPS: I. Exoplanet detection and candidates
DOI: 10.1051/0004-6361/202346570 Bibcode: 2024A&A...689A..32M

Bouchy, F.; Meunier, N.; Unger, N. +12 more

Context. The census of planets around M dwarfs in the solar neighbourhood meets two challenges: detecting the best targets for the future characterisation of planets with ELTs, and studying the statistics of planet occurrence that are crucial to formation scenarios. The radial velocity (RV) method remains the most appropriate for such a census as …

2024 Astronomy and Astrophysics
Gaia 1
Hints of a close outer companion to the ultra-hot Jupiter TOI-2109 b
DOI: 10.1051/0004-6361/202451068 Bibcode: 2024A&A...692A.254H

Alonso, R.; Deleuil, M.; Erikson, A. +86 more

Context. Hot Jupiters (HJs) with close-by planetary companions are rare, with only a handful of them having been discovered so far. This could be due to their suggested dynamical histories, which lead to the possible ejection of other planets. TOI-2109 b is special in this regard because it is the HJ with the closest relative separation from its h…

2024 Astronomy and Astrophysics
CHEOPS 1
Triple trouble with PSR J1618‑3921: Mass measurements and orbital dynamics of an eccentric millisecond pulsar
DOI: 10.1051/0004-6361/202347482 Bibcode: 2024A&A...691A..22G

Guillemot, L.; Possenti, A.; Kramer, M. +11 more

Context. PSR J1618‑3921 is one of five known millisecond pulsars (MSPs) in eccentric orbits (eMPSs) located in the Galactic plane, whose formation is poorly understood. Earlier studies of these objects revealed significant discrepancies between observations and predictions from standard binary evolution scenarios of pulsar-helium white dwarf (HeWD…

2024 Astronomy and Astrophysics
Gaia 1
Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares
DOI: 10.1051/0004-6361/202451838 Bibcode: 2024A&A...692A.176C

Krucker, Säm; Veronig, Astrid M.; Polito, Vanessa +10 more

Aims. This paper aims to demonstrate the importance of short-exposure extreme ultraviolet (EUV) observations of solar flares in the study of particle acceleration, heating, and energy partition in flares. This work highlights the observations now available from the Extreme Ultraviolet Imager (EUI) instrument suite on board Solar Orbiter while oper…

2024 Astronomy and Astrophysics
SolarOrbiter 1
J-PLUS: Bayesian object classification with a strum of BANNJOS
DOI: 10.1051/0004-6361/202450503 Bibcode: 2024A&A...691A.221D

Hernández-Monteagudo, C.; Hernán-Caballero, A.; Vázquez Ramió, H. +22 more

Context. With its 12 optical filters, the Javalambre-Photometric Local Universe Survey (J-PLUS) provides an unprecedented multicolor view of the local Universe. The third data release (DR3) covers 3192 deg2 and contains 47.4 million objects. However, the classification algorithms currently implemented in the J-PLUS pipeline are determin…

2024 Astronomy and Astrophysics
Gaia 1