Search Publications

Ice inventory towards the protostar Ced 110 IRS4 observed with the James Webb Space Telescope: Results from the Early Release Science Ice Age program
DOI: 10.1051/0004-6361/202451505 Bibcode: 2025A&A...693A.288R

Sun, F.; Egami, E.; van Dishoeck, E. F. +37 more

Context. Protostars contain icy ingredients necessary for the formation of potential habitable worlds, therefore, it is crucial to understand their chemical and physical environments. This work is focused on the ice features towards the binary protostellar system Ced 110 IRS4A and IRS4B, separated by 250 au and observed with James Webb Space Teles…

2025 Astronomy and Astrophysics
ISO 4
The Discovery and Characterization of Minimoon 2024 PT5
DOI: 10.3847/2041-8213/ada1d0 Bibcode: 2025ApJ...978L..37B

Chiboucas, Kristin; Lemaux, Brian C.; Bolin, Bryce T. +4 more

Minimoons are asteroids that become temporarily captured by the Earth–Moon system. We present the discovery of 2024 PT5, a minimoon discovered by the Asteroid Terrestrial-impact Last Alert System Sutherland telescope on 2024 August 7. The minimoon with heliocentric semimajor axis, a ~ 1.01 au, and perihelion, q ~ 0.99 au, became capture…

2025 The Astrophysical Journal
Gaia 4
Euclid: A complete Einstein ring in NGC 6505
DOI: 10.1051/0004-6361/202453014 Bibcode: 2025A&A...694A.145O

Altieri, B.; Aussel, H.; Cimatti, A. +195 more

We report the discovery of a complete Einstein ring around the elliptical galaxy NGC 6505, at z = 0.042. This is the first strong gravitational lens discovered in Euclid and the first in an NGC object from any survey. The combination of the low redshift of the lens galaxy, the brightness of the source galaxy (IE = 18.1 lensed, IE

2025 Astronomy and Astrophysics
EUCLID 4
Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-timescale Variables, and the Unusual Nucleus of WeSb 1
DOI: 10.1088/1538-3873/ada702 Bibcode: 2025PASP..137b4201B

Kulkarni, S. R.; Riddle, Reed; Kong, Albert K. H. +16 more

A complete understanding of the central stars of planetary nebulae (CSPNe) remains elusive. Over the past several decades, time-series photometry of CSPNe has yielded significant results including, but not limited to, discoveries of nearly 100 binary systems, insights into pulsations and winds in young white dwarfs, and studies of stars undergoing…

2025 Publications of the Astronomical Society of the Pacific
Gaia 4
The magnetic field of the Radcliffe wave: Starlight polarization at the nearest approach to the Sun
DOI: 10.1051/0004-6361/202450991 Bibcode: 2025A&A...694A..97P

Alves, J.; Panopoulou, G. V.; Soler, J. D. +6 more

Aims. We investigate the geometry of the magnetic field toward the Radcliffe wave, a coherent part of the nearby Local Arm of 3 kpc in length recently discovered via three-dimensional dust mapping. Methods. We used archival stellar polarization in the optical and new measurements in the near-infrared to trace the magnetic field as projected on the…

2025 Astronomy and Astrophysics
Gaia 4
Deeply comprehensive astrometric, photometric, and kinematic studies of the three OCSN open clusters with Gaia DR3
DOI: 10.1007/s12036-025-10044-0 Bibcode: 2025JApA...26...21E

Elsanhoury, W. H.; Çınar, D. C.; Haroon, A. A. +1 more

In this study, we considered the optical wavelength of Gaia Data Release 3 (DR3) to analyze poorly studied three newly open star clusters, namely OCSN 203, OCSN 213, and OCSN 244 clusters with ASTECA code. Here, we identified 227, 200, and 551 candidates with highly probable (P

2025 Journal of Astrophysics and Astronomy
Gaia 3
On Finding Black Holes in Photometric Microlensing Surveys
DOI: 10.3847/1538-4357/adb1d7 Bibcode: 2025ApJ...981..183K

Lu, Jessica R.; McGill, Peter; Dawson, William A. +5 more

There are expected to be millions of isolated black holes in the galaxy resulting from the deaths of massive stars. Measuring the abundance and properties of this remnant population would shed light on the end stages of stellar evolution and the evolution paths of black hole systems. Detecting isolated black holes is currently only possible via gr…

2025 The Astrophysical Journal
Gaia 3
Empirical Color Correction to MIST and PARSEC Isochrones on Gaia BR ‑ RP and G ‑ RP with Benchmark Open Clusters
DOI: 10.3847/1538-4357/ad960a Bibcode: 2025ApJ...979...92W

Fang, Min; Wang, Fan; Tian, Haijun +8 more

Recent literature reports a color deviation between observed Gaia color–magnitude diagrams (CMDs) and theoretical model isochrone predictions, particularly in the very low-mass regime. To assess its impact on cluster age determination via isochrone fitting, we quantified the color deviations for three benchmark clusters, Hyades, Pleiades, and Prae…

2025 The Astrophysical Journal
Gaia 3
Multiwavelength Constraints on the Local Black Hole Occupation Fraction
DOI: 10.3847/1538-4357/ad94d9 Bibcode: 2025ApJ...978...77B

Geha, Marla; Baldassare, Vivienne F.; Natarajan, Priyamvada +1 more

The fraction of dwarf galaxies hosting central, intermediate-mass black holes (IMBHs) at low redshifts is an important observational probe of black hole seeding at high redshift. Detections of nuclear accretion signatures in dwarf galaxies provides strong evidence for the presence of these IMBHs. We develop a Bayesian model to infer the black hole…

2025 The Astrophysical Journal
XMM-Newton 3
Dark Galactic Subhalos and the Gaia Snail
DOI: 10.3847/1538-4357/ada963 Bibcode: 2025ApJ...980...24G

Bovy, Jo; Benson, Andrew; Frankel, Neige +1 more

Gaia has revealed a clear signal of disequilibrium in the solar neighborhood in the form of a spiral (or snail) feature in the vertical phase-space distribution. We investigate the possibility that this structure emerges from ongoing perturbations by dark Galactic subhalos. We develop a probabilistic model for ge…

2025 The Astrophysical Journal
Gaia 3