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Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator
DOI: 10.1093/mnrasl/slae106 Bibcode: 2025MNRAS.536L..38V

Boccaletti, Anthony; Blouin, Simon; Pearce, Logan A. +3 more

We present the unplanned detection of a white dwarf companion to the star HD 218261 in mid-infrared (10-16 $\mu$m) observations with JWST/MIRI. This star was observed as a calibrator for coronagraphic observations of the exoplanet host HR 8799. HD 218261 B has only …

2025 Monthly Notices of the Royal Astronomical Society
Gaia 1
Martian hydrosphere: A brief overview of water on Mars
DOI: 10.1016/j.newar.2024.101714 Bibcode: 2025NewAR.10001714G

Gopalchetty, Brahma

Understanding the status of water on Mars is crucial for evaluating its capacity to support life and to serve as a resource for future possible human exploration. Investigations have been carried out in the past to find signs of water in its past or present states. It is generally agreed that Mars had significant amounts of water early in its exis…

2025 New Astronomy Reviews
MEx 1
A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-minute Period Variable Gaia22ayj
DOI: 10.1088/1538-3873/adb0f1 Bibcode: 2025PASP..137b4202R

Mori, Kaya; Riddle, Reed; Szkody, Paula +30 more

White dwarfs (WDs) are the most abundant compact objects, and recent surveys have suggested that over a third of WDs in accreting binaries host a strong (B ≳ 1 MG) magnetic field. However, the origin and evolution of WD magnetism remain under debate. Two WD pulsars, AR Sco and J191213.72–441045.1 (J1912), have been found, which are non-accreting b…

2025 Publications of the Astronomical Society of the Pacific
Gaia 1
MOCKA – A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators
DOI: 10.1051/0004-6361/202452811 Bibcode: 2025A&A...694A.185J

Aigrain, S.; Plachy, E.; De Ridder, J. +14 more

Context. With the PLAnetary Transits and Oscillation of stars (PLATO) space mission set for launch in December 2026 by the European Space Agency (ESA), a new photometric legacy and a future of new scientific discoveries await the community. By exploring scientific topics outside of the core science program, the PLATO complementary science program …

2025 Astronomy and Astrophysics
Gaia 1
Binary and grouped open clusters: A new catalogue
DOI: 10.1051/0004-6361/202452672 Bibcode: 2025A&A...693A.218P

Baume, G.; Feinstein, C.; Palma, T. +1 more

Context. Understanding the formation and evolution of star clusters in the Milky Way requires precise identification of clusters that form binary or multiple systems. Such systems offer valuable insight into the dynamical processes and interactions that influence cluster evolution. Aims. This study aims to detect and classify star clusters in the …

2025 Astronomy and Astrophysics
Gaia 1
Determining the Nature of IC 10 X-2: A Comprehensive Study of the Optical/IR Emission from an Extragalactic BeHMXB
DOI: 10.3847/1538-4357/ad82df Bibcode: 2025ApJ...978..170A

Gelfand, Joseph D.; Heinke, Craig; Lewis, Fraser +7 more

We present a comprehensive analysis of the optical and infrared (IR) properties of high-mass X-ray binary (HMXB) IC 10 X-2, classified as a supergiant HMXB and superfast X-ray transient by previous work. Our analysis of regular (daily and weekly) observations by both the Zwicky Transient Facility and Las Cumbres Observatory over a 5 yr period indi…

2025 The Astrophysical Journal
Gaia 1
The disrupting and growing open cluster spiral arm patterns of the Milky Way
DOI: 10.1093/mnras/staf153 Bibcode: 2025MNRAS.537.2403L

Luo, Yangping; Wang, Kun; Liu, Xiaochen +1 more

Star clusters provide unique advantages for investigating Galactic spiral arms, particularly due to their precise ages, positions, and kinematic properties, which are further enhanced by ongoing updates from the astrometric data. In this study, we employ the latest extensive catalogue of open clusters from Gaia DR3 to examine the positional deviat…

2025 Monthly Notices of the Royal Astronomical Society
Gaia 1
Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
DOI: 10.1051/0004-6361/202451300 Bibcode: 2025A&A...693A..90B

Fridlund, M.; Pallé, E.; Gandolfi, D. +38 more

Context. TOI-396 is an F6 V bright naked-eye star (V ≈ 6.4) orbited by three small (Rp ≈ 2 R) transiting planets discovered thanks to space-based photometry from two TESS sectors. The orbital periods of the two innermost planets, namely TOI-396 b and c, are close to the 5:3 commensurability (Pb ~ 3.6 d and Pc…

2025 Astronomy and Astrophysics
Gaia 1
Two Earth-size Planets and an Earth-size Candidate Transiting the nearby Star HD 101581
DOI: 10.3847/1538-3881/ad9266 Bibcode: 2025AJ....169...47K

Butler, R. Paul; Vanderburg, Andrew; Brahm, Rafael +43 more

We report the validation of multiple planets transiting the nearby (d = 12.8 pc) K5V dwarf HD 101581 (GJ 435, TOI–6276, TIC 397362481). This system consists of at least two Earth-size planets whose orbits are near a mutual 4:3 mean-motion resonance, HD 101581 b ( , P = 4.47 days) and HD 101581c (

2025 The Astronomical Journal
Gaia 1
Multi-wavelength study of 1eRASS J085039.9‑421151 with eROSITA, NuSTAR, and X-shooter
DOI: 10.1051/0004-6361/202348708 Bibcode: 2025A&A...693A.260Z

Santangelo, A.; Heber, U.; Dauser, T. +23 more

The eROSITA instrument on board Spectrum-Roentgen-Gamma (SRG) has completed four scans of the X-ray sky, leading to the detection of almost one million X-ray sources in eRASS1 alone, including multiple new X-ray binary candidates. We report on analysis of the X-ray binary 1eRASS J085039.9‑421151, using a ∼55 ks long NuSTAR observation, following i…

2025 Astronomy and Astrophysics
Gaia INTEGRAL 1