Search Publications

The AMBRE Project: Lead abundance in Galactic stars
DOI: 10.1051/0004-6361/202450782 Bibcode: 2024A&A...690A..97C

Recio-Blanco, A.; de Laverny, P.; Contursi, G. +4 more

Context. The chemical evolution of neutron capture elements in the Milky Way is still a matter of debate. Although more and more studies investigate their chemical behaviour, there is still a lack of a significant large sample of abundances of a key heavy element: lead. Aims. Lead is the final product of the s-process nucleosynthesis channel and i…

2024 Astronomy and Astrophysics
Gaia 0
Water ice concentration and distribution in the Martian south polar layered deposits constrained by the lateral variations of their bulk density
DOI: 10.1016/j.icarus.2024.116025 Bibcode: 2024Icar..41416025G

Mitri, Giuseppe; Genova, Antonio; Sulcanese, Davide +4 more

Records of Mars' climate history have been preserved by the ice-rich south polar layered deposits. An accurate knowledge of their properties is key to understanding the evolution of Mars. The combination of geophysical measurements, including gravity, altimetry and radar sounding, enables constraints on the density and composition of the south pol…

2024 Icarus
MEx 0
The Role and Lifetime of Dissociative Heterogeneous Processes in Improving Simulated Ozone on Mars
DOI: 10.1029/2024JE008302 Bibcode: 2024JGRE..12908302B

Patel, M. R.; Mason, J. P.; Lefèvre, F. +4 more

Ozone simulated in Mars Global Climate Models (MGCMs) is used to assess the underlying chemistry occurring in the atmosphere. Currently, ozone total column abundance (TCA) is under-predicted in MGCMs by up to 120%, implying missing or inaccurate chemistry in models. Heterogeneous reactions of hydroxyl radicals (HOX) have been offered as…

2024 Journal of Geophysical Research (Planets)
ExoMars-16 0
Are There Local Dynamos Acting in Sunspot Regions?
DOI: 10.3847/1538-4357/ad7820 Bibcode: 2024ApJ...975...46J

Wang, Jingxiu; Jin, Chunlan; Ji, Haisheng +1 more

In solar physics, a long-unanswered question is whether or not there are local dynamos acting in sunspot regions. Here we report an observed pattern of magnetic evolution that makes the sunspots alive with ample complexity and energy. This anomalous pattern manifests as peculiar bipolar magnetic emergences (BMEs), exhibiting the following characte…

2024 The Astrophysical Journal
Hinode SOHO 0
Cross-correlation of Luminous Red Galaxies with Machine Learning Selected Active Galactic Nuclei in HSC-SSP: Unobscured AGN Residing in More Massive Halos
DOI: 10.3847/1538-4357/ad8342 Bibcode: 2024ApJ...977..158C

Strauss, Michael A.; Greene, Jenny E.; Goulding, Andy D. +7 more

Active galactic nuclei (AGN) are the signposts of black hole growth, and likely play an important role in galaxy evolution. An outstanding question is whether AGN of different spectral types indicate different evolutionary stages in the coevolution of black holes and galaxies. We present the angular correlation function between an AGN sample selec…

2024 The Astrophysical Journal
Gaia 0
Atmospheric Parameters and Abundances of Cool Red Giant Stars
DOI: 10.1088/1538-3873/ad4177 Bibcode: 2024PASP..136e4202D

Dencs, Z.; Derekas, A.; Mitnyan, T. +10 more

Understanding the atmospheric parameters of stars on the top of the RGB is essential to reveal the chemical composition of the Milky Way, as they can be used to probe the farthest parts of our Galaxy. Our goal is to determine the chemical composition of 21 RGB stars with T eff < 4200 K selected from the APOGEE-2 DR17 database using n…

2024 Publications of the Astronomical Society of the Pacific
Gaia 0
European VLBI Network observations of the peculiar radio source 4C 35.06 overlapping with a compact group of nine galaxies
DOI: 10.1051/0004-6361/202348729 Bibcode: 2024A&A...684A.188V

An, T.; Gabányi, K. É.; Frey, S. +8 more

Context. According to the hierarchical structure formation model, brightest cluster galaxies (BCGs) evolve into the most luminous and massive galaxies in the Universe through multiple merger events. The peculiar radio source 4C 35.06 is located at the core of the galaxy cluster Abell 407, overlapping with a compact group of nine galaxies. Low-freq…

2024 Astronomy and Astrophysics
Gaia 0
WEAVE First Light Observations: Origin and Dynamics of the Shock Front in Stephan's Quintet
DOI: 10.1093/mnras/stae2235 Bibcode: 2024MNRAS.535.2269A

Shimwell, T. W.; Monguió, M.; Hardcastle, M. J. +62 more

We present a detailed study of the large-scale shock front in Stephan's Quintet, a by-product of past and ongoing interactions. Using integral-field spectroscopy from the new William Herschel Telescope Enhanced Area Velocity Explorer (WEAVE), recent 144 MHz observations from the LOFAR Two-metre Sky Survey, and archival data from the Very Large Arr…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 0
Constraining Quasar Feedback from Analysis of the Hydrostatic Equilibrium of the Molecular Gas in Their Host Galaxies
DOI: 10.3847/1538-4357/ad7e26 Bibcode: 2024ApJ...976..201F

Ho, Luis C.; Bauer, Franz E.; Treister, Ezequiel +4 more

We investigate the kinematics and dynamics of the molecular and ionized gas in the host galaxies of three Palomar-Green quasars at low redshifts, benefiting from the archival millimeter-wave interferometric and optical integral field unit data. We study the kinematics of both cold molecular and hot ionized gas by analyzing the CO and Hα data cubes…

2024 The Astrophysical Journal
eHST 0
Studying the Kinematics of the Stellar Association TW Hya from Current Data
DOI: 10.1134/S1990341324600443 Bibcode: 2024AstBu..79..473B

Bobylev, V. V.; Bajkova, A. T.

The kinematics of the young stellar association near the Sun TW Hya is studied. Kinematic estimates of the age of this association were obtained in two ways. The first method—the analysis of stellar trajectories integrated back in time—gave an estimate of the age $$t=4.9\pm 1.2$$

2024 Astrophysical Bulletin
Gaia 0