Search Publications

SWEET-Cat: A view on the planetary mass-radius relation
DOI: 10.1051/0004-6361/202451704 Bibcode: 2024A&A...691A..53S

Adibekyan, V.; Hoyer, S.; Sousa, S. G. +9 more

Aims. SWEET-Cat (Stars With ExoplanETs Catalog) was originally introduced in 2013, and since then, the number of confirmed exoplanets has increased significantly. A crucial step for a comprehensive understanding of these new worlds is the precise and homogeneous characterization of their host stars. Methods. We used a large number of high-resoluti…

2024 Astronomy and Astrophysics
Gaia 1
Icarus Revisited: An Ancient, Metal-poor Accreted Stellar Stream in the Disk of the Milky Way
DOI: 10.3847/1538-4357/ad8887 Bibcode: 2024ApJ...977..278R

Vitali, Sara; Cignoni, Michele; Lattanzi, Mario G. +2 more

The search for accreted satellites in the Galactic disk is a challenging task, to which Gaia plays a crucial role in synergy with ground-based spectroscopic surveys. In 2021, P. Re Fiorentin et al. discovered five substructures with disk kinematics including Icarus. To gain more insight into the origin of Icarus as a remnant of a dwarf galaxy rath…

2024 The Astrophysical Journal
Gaia 1
The restless population of bright X-ray sources of NGC 3621
DOI: 10.1051/0004-6361/202450319 Bibcode: 2024A&A...689A.217S

Salvaterra, R.; Tiengo, A.; Marelli, M. +9 more

We report on the multi-year evolution of the population of X-ray sources in the nuclear region of NGC 3621 based on Chandra, XMM-Newton, and Swift observations. Among these, two sources, X1 and X5, after their first detection in 2008, seem to have faded below the detectability threshold, a most interesting fact as X1 is associated with the active …

2024 Astronomy and Astrophysics
XMM-Newton 1
COSMOS brightest group galaxies: III. Evolution of stellar ages
DOI: 10.1051/0004-6361/202449543 Bibcode: 2024A&A...690A.315G

Finoguenov, A.; Ilbert, O.; Magdis, G. E. +15 more

The unique characteristics of the brightest group galaxies (BGGs) serve as a link in the evolutionary continuum between galaxies such as the Milky Way and the more massive brightest cluster galaxies found in dense clusters. This research investigates the evolution of the stellar properties of BGGs over cosmic time (z = 0.08 ‑ 1.30), extending the …

2024 Astronomy and Astrophysics
eHST 1
Multipoint observations of compressional Pc5-6 pulsations in the dawn side magnetosphere: A case study
DOI: 10.1016/j.asr.2023.10.018 Bibcode: 2024AdSpR..73..597K

Sibeck, D. G.; Korotova, G. I.

We present a case study of compressional Pc5-6 pulsations observed by THEMIS-D and -E in the dawn sector of the magnetosphere following 1100 UT on January 22, 2010. The pulsations were observed during a moderate substorm triggered by the IMF discontinuity and an accompanying change in the solar wind dynamic pressure at 1045 UT. The event can be co…

2024 Advances in Space Research
Cluster 1
Testing the flux tube expansion factor - solar wind speed relation with Solar Orbiter data
DOI: 10.1051/0004-6361/202451272 Bibcode: 2024A&A...691A..77D

Maksimovic, M.; Louarn, P.; Démoulin, P. +5 more

Context. The properties of the solar wind measured in situ in the heliosphere are largely controlled by energy deposition in the solar corona, which is in turn closely related to the properties of the coronal magnetic field. Previous studies have shown that long-duration and large-scale magnetic structures show an inverse relation between the sola…

2024 Astronomy and Astrophysics
SolarOrbiter 1
Radial Metallicity Gradients for the Chemically Selected Galactic Thin Disc Main-Sequence Stars
DOI: 10.1002/asna.20240052 Bibcode: 2024AN....34540052A

Seabroke, G. M.; Bilir, S.; Ak, T. +3 more

We present the radial metallicity gradients within the Galactic thin disc population through main-sequence stars selected on the chemical plane using GALAH DR3 accompanied with Gaia DR3 astrometric data. The [Fe/H], [α/Fe] and [Mg/H] radial gradients are estimated for guiding radius as -0.074±0.006, +0.004±0.002, -0.074±0.006 dex kpc -1

2024 Astronomische Nachrichten
Gaia 1
Discovery of Two Different Full Disk Evolutionary Patterns of M-type T Tauri Stars with LAMOST DR8
DOI: 10.3847/1538-4357/ad04d3 Bibcode: 2024ApJ...960...58H

Zhao, Yongheng; Duan, Fuqing; Li, Guang-Wei +2 more

The full disk, full of gas and dust, determines the upper limit of planet masses, and its lifetime is critical for planet formation, especially for giant planets. In this work, we studied the evolutionary timescales of the full disks of T Tauri stars (TTSs) and their relations to accretion. Combined with Gaia EDR3, Two Micron All Sky Survey, and W…

2024 The Astrophysical Journal
Gaia 1
PeVatron candidate SNR G106.3+2.7 in a low-density cavity: a multiwavelength test
DOI: 10.1093/mnras/stae058 Bibcode: 2024MNRAS.528.5487B

Liu, Ruo-Yu; Chen, Yang; Ge, Chong +1 more

In this paper, we constrain the density of the interstellar medium (ISM) around the hadronic PeVatron candidate, supernova remnant (SNR) G106.3+2.7, based on X-ray and γ-ray observations. The purpose of this investigation is to understand the influence of the gaseous environment on this SNR as a proton PeVatron candidate. By modelling the self-reg…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
Telescope control software and proto-model siderostat for the SDSS-V Local Volume Mapper
DOI: 10.1117/1.JATIS.10.3.037001 Bibcode: 2024JATIS..10c7001A

Kollmeier, Juna A.; Drory, Niv; Froning, Cynthia S. +19 more

The fifth Sloan Digital Sky Survey Local Volume Mapper (LVM) is a wide-field integral field unit survey that uses an array of four 160 mm fixed telescopes with siderostats to minimize the number of moving parts. An individual telescope observes the science or calibration field independently and is synchronized with the science exposure. We develop…

2024 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 1