Search Publications

Localizing short-period pulsations in hard X-rays and γ-rays during an X9.0 flare
DOI: 10.1051/0004-6361/202453613 Bibcode: 2025A&A...695L...4L

Li, Dong

Context. The feature of quasi-periodic pulsations (QPPs) is frequently observed in the light curve of solar and stellar flares. However, the short-period QPP is rarely reported in the high energy range of hard X-rays (HXRs) and γ-rays. Aims. We investigated the QPP at a shorter period of about 1 s in high-energy channels of HXRs and γ-ray continuu…

2025 Astronomy and Astrophysics
SolarOrbiter 1
The cosmological analysis of X-ray cluster surveys: VI. Inference based on analytically simulated observable diagrams
DOI: 10.1051/0004-6361/202450499 Bibcode: 2025A&A...693A..46K

Pierre, M.; Werner, N.; Kosiba, M. +4 more

Context. The number density of galaxy clusters across mass and redshift has been established as a powerful cosmological probe, yielding important information on the matter components of the Universe. Cosmological analyses with galaxy clusters traditionally employ scaling relations, which are empirical relationships between cluster masses and their…

2025 Astronomy and Astrophysics
XMM-Newton 1
Development and Evolution of Icy Layer Outcrops on Mars' North Polar Ice Cap: Observations of Vertical and Lateral Variability
DOI: 10.1029/2024JE008377 Bibcode: 2025JGRE..13008377P

Mustard, John F.; Becerra, Patricio; Bramson, Ali M. +1 more

Mars' north polar ice cap features troughs that cut into the ice, exposing subsurface layers of different brightness and topographic expression. Specifically, these layers represent two different stratum types: lower albedo (higher dust content) marker beds, which protrude out of the wall topographically, and higher albedo (i.e., icier) interbeds,…

2025 Journal of Geophysical Research (Planets)
MEx 1
Unveiling the Origins and Dynamics of the Hierarchical Triple Star System CN Lyn
DOI: 10.3847/1538-3881/ad9d46 Bibcode: 2025AJ....169...71Y

Bakış, Volkan; Bilir, Selçuk; Alan, Neslihan +3 more

In this study, we present a detailed analysis of CN Lyn, an overlooked triple star system, by combining spectroscopic data from the literature, photometric Transiting Exoplanet Survey Satellite data, and kinematic techniques. We updated the fundamental parameters of the known eclipsing components in the system with high precision. The chemical com…

2025 The Astronomical Journal
Gaia 1
Direct N-body simulations of NGC 6397 and its tidal tails
DOI: 10.1093/mnras/staf121 Bibcode: 2025MNRAS.537.1807A

Baumgardt, Holger; Arnold, Anthony D.

We have performed a series of direct N-body simulations that study the evolution of the Galactic globular cluster NGC 6397 under the combined influence of two-body relaxation, stellar evolution, and the Milky Way's tidal field. Our simulations follow the evolution of the cluster over the last several Gyr up to its present-day position in the Milky…

2025 Monthly Notices of the Royal Astronomical Society
Gaia 1
Metallicity Dependence of Giant Planets around M Dwarfs
DOI: 10.3847/1538-4365/ad9c65 Bibcode: 2025ApJS..276...47G

Burgasser, Adam J.; Gan, Tianjun; Mao, Shude +2 more

We investigate the stellar metallicity ([Fe/H] and [M/H]) dependence of giant planets around M dwarfs by comparing the metallicity distribution of 746 field M dwarfs without known giant planets with a sample of 22 M dwarfs hosting confirmed giant planets. All metallicity measurements are homogeneously obtained through the same methodology based on…

2025 The Astrophysical Journal Supplement Series
Gaia 1
A study of the frequency and characteristics of stellar companions and Jupiter-like planets in nearby open clusters
DOI: 10.1051/0004-6361/202452253 Bibcode: 2025A&A...694A.175G

Barbato, D.; D'Orazi, V.; Nascimbeni, V. +9 more

Context. Observations of companions of solar-type stars in nearby young moving groups (NYMGs) show that they split into two groups: stellar and brown dwarf companions (mass ratio q > 0.05) and Jupiter-like (JL) planets (q < 0.02). The frequency of JL planets in NYMGs appears to be higher than that obtained from radial velocity (RV) surveys. …

2025 Astronomy and Astrophysics
Gaia 1
Behind the dust veil: A panchromatic view of an optically dark galaxy at z = 4.82
DOI: 10.1051/0004-6361/202452932 Bibcode: 2025A&A...693A.309S

Koekemoer, Anton M.; Daddi, Emanuele; Schinnerer, Eva +30 more

Optically dark dusty star-forming galaxies (DSFGs) play an essential role in massive galaxy formation at early cosmic time; however, their nature remains elusive. Here, we present a detailed case study of all the baryonic components of a z = 4.821 DSFG, XS55. Selected from the ultra-deep COSMOS-XS 3 GHz map with a red SCUBA-2 450 µm/850 &mic…

2025 Astronomy and Astrophysics
XMM-Newton 1
TESS Hunt for Young and Maturing Exoplanets (THYME). XII. A Young Mini-Neptune on the Upper Edge of the Radius Valley in the Hyades Cluster
DOI: 10.3847/1538-3881/ada26a Bibcode: 2025AJ....169..166D

Vanderburg, Andrew; Quinn, Samuel N.; Howell, Steve B. +19 more

We present the discovery and characterization of TOI-4364b, a young mini-Neptune in the tidal tails of the Hyades cluster, identified through TESS transit observations and ground-based follow-up photometry. The planet orbits a bright M dwarf (K = 9.1 mag) at a distance of 44 pc, with an orbital period of 5.42 days and an equilibrium temperature of…

2025 The Astronomical Journal
Gaia 1
Multiple Populations of the Large Magellanic Cloud Globular Cluster NGC 2257: No Major Environmental Effect on the Formation of Multiple Populations of Old Globular Clusters in the Large Magellanic Cloud
DOI: 10.3847/1538-3881/ada94e Bibcode: 2025AJ....169..143L

Kim, Hwihyun; Kim, Hak-Sub; Lee, Jae-Woo +3 more

How the environment of the host galaxy affects the formation of multiple populations (MPs) in globular clusters (GCs) is one of the outstanding questions in near-field cosmology. To understand the true nature of the old GC MPs in the Large Magellanic Cloud (LMC), we study the Ca–CN–CH photometry of the old metal-poor LMC GC NGC 2257. We find the p…

2025 The Astronomical Journal
Gaia 1