Search Publications

Equilibrium dynamical models in the inner region of the Large Magellanic Cloud based on Gaia DR3 kinematics
DOI: 10.1051/0004-6361/202451578 Bibcode: 2024A&A...692A..40K

Kacharov, Nikolay; van de Ven, Glenn; Khoperskov, Sergey +3 more

Context. The Large Magellanic Cloud (LMC) contains complex dynamics driven by both internal and external processes. The external forces are due to tidal interactions with the Small Magellanic Cloud and the Milky Way, while internally its dynamics mainly depend on the stellar, gas, and dark matter mass distributions. Despite this complexity, simple…

2024 Astronomy and Astrophysics
Gaia 6
Satellite group infall into the Milky Way: Exploring the Crater-Leo case with new HST proper motions
DOI: 10.1051/0004-6361/202449985 Bibcode: 2024A&A...687A.212J

van der Marel, Roeland P.; Pawlowski, Marcel S.; Júlio, Mariana P. +3 more

Context. Within Λ cold dark matter (ΛCDM) simulations, Milky Way-like galaxies accrete some of their satellite galaxies in groups of 3–5 members rather than individually, and this has been suggested as a possible mechanism driving the formation of satellite planes. Objects accreted in groups are expected to share similar specific total energy and …

2024 Astronomy and Astrophysics
eHST 6
El Gordo needs El Anzuelo: Probing the structure of cluster members with multi-band extended arcs in JWST data
DOI: 10.1051/0004-6361/202449876 Bibcode: 2024A&A...689A.304G

Caminha, G. B.; Suyu, S. H.; Galan, A. +2 more

Gravitational lensing by galaxy clusters involves hundreds of galaxies over a large redshift range and increases the likelihood of rare phenomena (supernovae, microlensing, dark substructures, etc.). Characterizing the mass and light distributions of foreground and background objects often requires a combination of high-resolution data and advance…

2024 Astronomy and Astrophysics
Gaia eHST JWST 6
SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first five surveys
DOI: 10.1051/0004-6361/202348950 Bibcode: 2024A&A...687A.183S

Sunyaev, R.; Krivonos, R.; Sazonov, S. +27 more

We present an updated catalog of sources detected by the Mikhail Pavlinsky ART-XC telescope aboard the Spektrum-Roentgen-Gamma (SRG) observatory during its all-sky survey. It is based on the data of the first four and the partially completed fifth scans of the sky (ARTSS1-5). The catalog comprises 1545 sources detected in the 4-12 keV energy band.…

2024 Astronomy and Astrophysics
Gaia INTEGRAL XMM-Newton 6
Identification of new nearby white dwarfs using Gaia DR3
DOI: 10.1051/0004-6361/202347767 Bibcode: 2024A&A...683A..33G

Reffert, Sabine; Golovin, Alex; Vani, Akash +3 more

Context. A volume-complete sample of white dwarfs is essential for statistical studies of the white dwarf population. The sample of nearby white dwarfs is the only one that allows the faint end of the luminosity function to be probed and thus is the only one that covers the entire range of white dwarf ages. However, due to their intrinsic faintnes…

2024 Astronomy and Astrophysics
Gaia 6
The IACOB project. XI. No increase in mass-loss rates over the bistability region
DOI: 10.1051/0004-6361/202450301 Bibcode: 2024A&A...687L..16D

Simón-Díaz, S.; Urbaneja, M. A.; de Burgos, A. +1 more

The properties of blue supergiants are key for constraining the end of the main sequence (MS) of massive stars. Whether the observed drop in the relative number of fast-rotating stars below ≈21 kK is due to enhanced mass-loss rates at the location of the bistability jump, or the result of the end of the MS is still debated. Here, we combine newly …

2024 Astronomy and Astrophysics
Gaia 6
TOI-4438 b: a transiting mini-Neptune amenable to atmospheric characterization
DOI: 10.1051/0004-6361/202349133 Bibcode: 2024A&A...685A.147G

Nagel, E.; Amado, P. J.; Caballero, J. A. +47 more

We report the confirmation and mass determination of a mini-Neptune transiting the M3.5 V star TOI-4438 (G 182-34) every 7.44 days. A transit signal was detected with NASA's TESS space mission in the sectors 40, 52, and 53. In order to validate the planet TOI-4438 b and to determine the system properties, we combined TESS data with high-precision …

2024 Astronomy and Astrophysics
Gaia 6
OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system
DOI: 10.1051/0004-6361/202348791 Bibcode: 2024A&A...685A..16H

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +32 more


Aims: Light curves of microlensing events occasionally deviate from the smooth and symmetric form of a single-lens single-source event. While most of these anomalous events can be accounted for by employing a binary-lens single-source (2L 1S) or a single-lens binary-source (1L2S) framework, it is established that a small fraction of events re…

2024 Astronomy and Astrophysics
eHST 6
Disruption of a massive molecular cloud by a supernova in the Galactic Centre: Initial results from the ACES project
DOI: 10.1051/0004-6361/202451190 Bibcode: 2024A&A...691A..70N

Immer, K.; Klessen, R. S.; Wang, Q. D. +33 more

The Milky Way's Central Molecular Zone (CMZ) differs dramatically from our local solar neighbourhood, both in the extreme interstellar medium conditions it exhibits (e.g. high gas, stellar, and feedback density) and in the strong dynamics at play (e.g. due to shear and gas influx along the bar). Consequently, it is likely that there are large-scal…

2024 Astronomy and Astrophysics
Herschel 6
PEWDD: A database of white dwarfs enriched by exo-planetary material
DOI: 10.1051/0004-6361/202450509 Bibcode: 2024A&A...691A.352W

Gänsicke, B. T.; Cunningham, T.; Izquierdo, P. +4 more

We present the Planetary Enriched White Dwarf Database (PEWDD), a collection of published photospheric abundances of white dwarfs accreting planetary debris alongside additional information relevant to metal-enrichment and the presence of infrared excesses, emission lines, and binary companions. At the time of publishing, PEWDD contains informatio…

2024 Astronomy and Astrophysics
Gaia 6