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Element abundances of galactic RGB stars in the APO-K2 catalogue: Dissimilarity in the scaling with [α/Fe]
DOI: 10.1051/0004-6361/202449755 Bibcode: 2024A&A...689A.159V

Valle, G.; Dell'Omodarme, M.; Prada Moroni, P. G. +1 more

Aims. We conducted an investigation on the chemical abundances of 4316 stars in the red giant branch (RGB) phase from the recently released APO-K2 catalogue. Our aim was to characterize the abundance trends of the single elements with [α/Fe], mainly focusing on C, N, and O, which are the most relevant for the estimation of stellar ages. Methods. T…

2024 Astronomy and Astrophysics
Gaia 1
A patchy CO2 exosphere on Ganymede revealed by the James Webb Space Telescope
DOI: 10.1051/0004-6361/202451599 Bibcode: 2024A&A...690L..11B

Leblanc, François; de Pater, Imke; Wong, Michael H. +25 more

Jupiter's icy moon Ganymede has a tenuous exosphere produced by sputtering and possibly sublimation of water ice. To date, only atomic hydrogen and oxygen have been directly detected in this exosphere. Here, we present observations of Ganymede's CO2 exosphere obtained with the James Webb Space Telescope. CO2 gas is observed o…

2024 Astronomy and Astrophysics
JWST 1
Geological Record of Water and Wind Processes on Mars as Observed by the Mars Express High Resolution Stereo Camera
DOI: 10.1007/s11214-024-01076-z Bibcode: 2024SSRv..220...45J

Jaumann, R.; Tirsch, D.; Hiesinger, H. +9 more

This review paper summarizes the observations and results of the Mars Express Mission and its application in the analysis of geological processes and landforms on Mars during the last 20 years. The Mars Express observations provided an extended data base allowing a comparative evaluation of different geological surface landforms and their time-bas…

2024 Space Science Reviews
MEx 1
Closeby Habitable Exoplanet Survey (CHES). II. An Observation Strategy for the Target Stars
DOI: 10.3847/1538-3881/ad6f01 Bibcode: 2024AJ....168..172T

Zhu, Zi; Li, Dong; Chen, Guo +11 more

The Closeby Habitable Exoplanet Survey (CHES) constitutes a mission intricately designed to systematically survey approximately 100 solar-type stars located within the immediate proximity of the solar system, specifically within a range of 10 pc. The core objective of this mission is the detection and characterization of potentially habitable Eart…

2024 The Astronomical Journal
Gaia 1
Relative alignments between magnetic fields, velocity gradients, and dust emission gradients in NGC 1333
DOI: 10.1093/mnras/stae1829 Bibcode: 2024MNRAS.533.1938C

Pattle, Kate; Karoly, Janik; Bastien, Pierre +24 more

Magnetic fields play an important role in shaping and regulating star formation in molecular clouds. Here, we present one of the first studies examining the relative orientations between magnetic (B) fields and the dust emission, gas column density, and velocity centroid gradients on the 0.02 pc (core) scales, using the BISTRO and VLA+GBT observat…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 1
Detection of Faint Sources by the UltraViolet Imaging Telescope Onboard AstroSat Using Poisson Distribution of Background
DOI: 10.3847/1538-3881/ad4991 Bibcode: 2024AJ....168...22A

Sreekumar, P.; Ananthamoorthy, B.; Bhattacharya, Debbijoy +1 more

We present an improved approach for constructing the UV source catalogs using observations from the UltraViolet Imaging Telescope (UVIT) onboard AstroSat, by considering the Poisson distribution of the UV background. The method is tested extensively using fields that are not crowded, the Small Magellanic Cloud and M31 (Field 13). The results are c…

2024 The Astronomical Journal
Gaia eHST 1
Determining the dynamical age of the LMC globular cluster NGC 1835 using the `dynamical clock'. Star density profile and blue straggler stars
DOI: 10.1051/0004-6361/202450088 Bibcode: 2024A&A...687A.310G

Vesperini, Enrico; Cadelano, Mario; Pallanca, Cristina +5 more

In the context of the study of the size-age relationship observed in star clusters in the Large Magellanic Cloud (LMC) and the investigation of its origin, we present the determination of the structural parameters and the dynamical age of the massive cluster NGC 1835. We used the powerful combination of optical and near-ultraviolet images acquired…

2024 Astronomy and Astrophysics
Gaia eHST 1
First Results of Mars Express—ExoMars Trace Gas Orbiter Mutual Radio Occultation
DOI: 10.1029/2023RS007873 Bibcode: 2024RaSc...5907873P

Cardesín-Moinelo, Alejandro; Wilson, Colin; Witasse, Olivier +10 more

Spacecraft-to-spacecraft radio occultations experiments are being conducted at Mars between Mars Express (MEX) and Trace Gas Orbiter (TGO), the first ever extensive inter-spacecraft occultations at a planet other than Earth. Here we present results from the first 83 such occultations, conducted between 2 Nov 2020 and 5th of July 2023. Of these, 44…

2024 Radio Science
ExoMars-16 MEx 1
First detection of X-ray pulsations and spectrum of the high Galactic latitude pulsar PSR J0837–2454 and direct Urca cooling implications
DOI: 10.1017/pasa.2024.64 Bibcode: 2024PASA...41...66H

Deller, Adam T.; Ho, Wynn C. G.; Becker, Werner +2 more

PSR J0837 $-$ 2454 is a young 629 ms radio pulsar whose uncertain distance has important implications. A large distance would place the pulsar far out of the Galactic plane and suggest it is the result of a runaway star, while a short distance would mean the pulsar is extraordinarily cold. He…

2024 Publications of the Astronomical Society of Australia
XMM-Newton 1
Fast X-ray/IR observations of the black hole transient Swift J1753.5–0127: From an IR lead to a very long jet lag
DOI: 10.1051/0004-6361/202450545 Bibcode: 2024A&A...690A.239U

Melandri, A.; Maccarone, T. J.; Altamirano, D. +16 more

We report two epochs of simultaneous near-infrared (IR) and X-ray observations of the low-mass X-ray binary black hole candidate Swift J1753.5–0127 with a subsecond time resolution during its long 2005–2016 outburst. Data were collected strictly simultaneously with VLT/ISAAC (KS band, 2.2 µm) and RXTE (2–15 keV) or XMM-Newton (0.7…

2024 Astronomy and Astrophysics
XMM-Newton 1