Search Publications

Testing Cluster Membership of Planetary Nebulae with High-precision Proper Motions. II. HST Observations of PHR J1315–6555 in the Open Cluster AL 1 (ESO 96-SC04)
DOI: 10.3847/1538-3881/adb034 Bibcode: 2025AJ....169..199B

Bond, Howard E.; Sahu, Kailash C.; Bellini, Andrea

Planetary nebulae (PNe) shown to be members of star clusters provide information on their properties and evolutionary histories that cannot be determined for PNe in the field, in particular the initial masses of their progenitor stars. Here we investigate the bipolar PN PHR J1315‑6555 (hereafter PHR J1315), which lies near the open cluster AL 1 (E…

2025 The Astronomical Journal
Gaia 1
Candidate RR Lyrae Associated with the Ultrafaint Dwarf Galaxy Aquarius III
DOI: 10.3847/1538-3881/adadf1 Bibcode: 2025AJ....169..156N

Ngeow, Chow-Choong; Bhardwaj, Anupam

We report the search of RR Lyrae in the vicinity of a newly discovered ultrafaint dwarf galaxy, Aquarius III. Based on the known RR Lyrae catalogs and gri-band light curves retrieved from public archives, we identified a RR Lyrae with distance, metallicity, and proper motion consistent with Aquarius III. Therefore, this RR Lyrae is the first varia…

2025 The Astronomical Journal
Gaia 1
Precise Orbit Determination of Mars-crossing Asteroids
DOI: 10.3847/1538-3881/ad8d57 Bibcode: 2025AJ....169...33L

Liu, Xin; Hou, Xi-Yun; Yao, Jun +4 more

This study investigates the orbit determination of the Mars-crossing asteroids (MCAs) with a focus on the possibility of detecting their Yarkovsky signals. We analyze the influences of force model uncertainties on MCA orbits, including the uncertainty of the main asteroid belt, and the uncertainty of the major planets' ephemeris. The main asteroid…

2025 The Astronomical Journal
Gaia 0
Resolving Pleiades Binary Stars with Gaia and Speckle Interferometric Observations
DOI: 10.3847/1538-3881/ada564 Bibcode: 2025AJ....169..145C

Chulkov, Dmitry; Strakhov, Ivan; Safonov, Boris

The Pleiades is the most prominent open star cluster visible from Earth and an important benchmark for simple stellar populations unified by common origin, age, and distance. Binary stars are its essential ingredient, yet their contribution remains uncertain due to heavy observational biases. A resolved multiplicity survey was conducted for a magn…

2025 The Astronomical Journal
Gaia 0
starkiller: Subtracting Stars and Other Sources from IFU Spectroscopic Data Through Forward Modeling
DOI: 10.3847/1538-3881/ad9f2b Bibcode: 2025AJ....169..148R

Bannister, Michele T.; Nordlander, Thomas; Ridden-Harper, Ryan +1 more

We present starkiller, an open-source Python package for forward-modeling flux retrieval from integral field unit (IFU) spectrograph data cubes. starkiller simultaneously provides stellar spectral classification, relative velocity, and line-of-sight extinction for all sources in a catalog, alongside a source-subtracted data cube. It performs synth…

2025 The Astronomical Journal
Gaia 0
Characterizing Superflares in HR 1099 Using Temporal and Spectral Analysis of XMM-Newton Observations
DOI: 10.3847/1538-3881/ad9601 Bibcode: 2025AJ....169...49D

Srivastava, A. K.; Pandey, Jeewan C.; Didel, Shweta

In the present paper, we analyze three energetic X-ray flares from the active RS CVn binary HR 1099 using data obtained from XMM-Newton. The flare duration ranges from 2.8 to 4.1 hr, with e-folding rise and decay times in the range of 27–38 minutes and 1.3–2.4 hr, respectively, indicating rapid rise and slower decay phases. The flare frequency for…

2025 The Astronomical Journal
XMM-Newton 0
A Bayesian Approach to Inferring Accretion Signatures in Young Stellar Objects: A Case Study with VIRUS
DOI: 10.3847/1538-3881/adadfa Bibcode: 2025AJ....169..155W

Mahadevan, Suvrath; Janowiecki, Steven; Zeimann, Gregory R. +3 more

The mass accretion rates of young stellar objects (YSOs) are key to understanding how stars form, how their circumstellar disks evolve, and even how planets form. We develop a Bayesian framework to determine the accretion rates of a sample of 15 YSOs using archival data from the VIRUS spectrograph (R ∼ 800, 3500–5500 Å) on the Hobby–Eberly Telesco…

2025 The Astronomical Journal
Gaia 0
Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST
DOI: 10.3847/1538-3881/ad9915 Bibcode: 2025AJ....169...60H

Han, Zhanwen; Kovalev, Mikhail; Chen, Xuefei +8 more

Triple star systems are critical for understanding stellar dynamics and compact objects in astrophysics, yet confirmed hierarchical triples identified via spectroscopy remain limited. In this study, we identified 23 triple systems by cross matching the Gaia DR3 non-single-star catalog with Large Sky Area Multi-Object Fiber Spectroscopic Telescope …

2025 The Astronomical Journal
Gaia 0
New Ultracool Companions to Nearby White Dwarfs
DOI: 10.3847/1538-3881/ad9b9b Bibcode: 2025AJ....169..100B

Debes, John H.; Meisner, Aaron M.; Kirkpatrick, J. Davy +15 more

We conducted a search for new ultracool companions to nearby white dwarfs using multiple methods, including the analysis of colors and examination of images in both the optical and the infrared. Through this process, we identified 51 previously unrecognized systems with candidate ultracool companions. 31 of these systems are resolved in at least o…

2025 The Astronomical Journal
Gaia 0
A Centroiding Algorithm for Point-source Trails
DOI: 10.3847/1538-3881/adb3a3 Bibcode: 2025AJ....169..183W

Rambaux, Nicolas; Lainey, Valéry; Cooper, Nick +3 more

Astrometric measurements are significantly challenged by the relative motion between the point source and the telescope, primarily due to the difficulty in accurately determining the position of the point source at the mid-exposure moment. Especially when the trail is irregular in shape or results from nonuniform relative motion, determining the c…

2025 The Astronomical Journal
Gaia 0