Search Publications

Calibrating the Color–Magnitude Relation of M Giants by Using Open Clusters
DOI: 10.3847/1538-4365/ad9f39 Bibcode: 2025ApJS..276...63T

Hao, C. J.; Xu, Y.; Lin, Z. H. +8 more

M giants, with their distinctive properties such as high luminosity, serve as excellent indicators for mapping the structure of the Milky Way. The distance to distant M giants can be determined by using the color–magnitude relation (CMR), which is derived from color–magnitude diagrams of specific systems in previous studies. In this work, we aimed…

2025 The Astrophysical Journal Supplement Series
Gaia 0
Chemodynamic evolution of Sun-like stars in nearby moving groups
DOI: 10.1093/mnras/stae2656 Bibcode: 2025MNRAS.536..498L

Murphy, Michael T.; Liu, Fan; Flynn, Chris +1 more

Sun-like stars are well represented in the solar neighbourhood but are currently underutilized, with many studies of chemical and kinematic evolution focusing on red giants (which can be observed further away) or turn-off stars (which have well-measured ages). Recent surveys (e.g. GALAH) provide spectra for large numbers of nearby Sun-like stars, …

2025 Monthly Notices of the Royal Astronomical Society
Gaia 0
Geomorphological study of the gullies in Penticton Crater, Mars: Classification and origin
DOI: 10.1016/j.pss.2024.106014 Bibcode: 2025P&SS..25506014N

Natarajan, Varsha; K N, Kusuma; Nandana, D. Lekshmi

Penticton crater, a southern hemisphere mid-latitude crater on Mars, is covered with features that are typical examples of Martian gullies that resemble the terrestrial gullies on Earth. We studied the gullies present in the Penticton crater, classified them and interpreted their formation mechanism using a remote sensing approach. A wide variety …

2025 Planetary and Space Science
MEx 0
A study on the evolutionary period changes of short-period type II cepheids
DOI: 10.1007/s10509-025-04418-7 Bibcode: 2025Ap&SS.370...28Y

Pastukhova, Elena N.; Yacob, Alemiye Mamo; Berdinkov, Leonid N.

We investigate the period changes of 13 short-period Type II Cepheids using the O-C method over a century-long data baseline. The O-C diagrams for these stars exhibit a parabolic trend, indicating both increasing and decreasing period changes over time. These observed period changes are consistent with recent theoretical models based on horizontal…

2025 Astrophysics and Space Science
INTEGRAL 0
Short-wave fadeout on mars: Radio absorption in the dayside martian ionosphere enhanced by solar flares
DOI: 10.1016/j.icarus.2024.116342 Bibcode: 2025Icar..42516342H

Lester, M.; Sánchez-Cano, B.; Harada, Y. +1 more

Solar flares can cause radio absorption in the D region of the Earth's ionosphere and consequently interrupt high-frequency radio communication systems, also known as short-wave fadeout or the Dellinger effect. We present an analogous radio absorption event observed at Mars during a solar flare. In this event, the Mars Express Mars Advanced Radar …

2025 Icarus
MEx 0
How inclusion of binaries affects the fitting of giant branches and determination of fundamental parameters of star clusters
DOI: 10.1016/j.newast.2024.102342 Bibcode: 2025NewA..11602342Z

Li, Zhongmu; Zhou, Yun

Open clusters (OCs) play an important role in the study of star formation and the structural evolution of the Milky Way. This paper fits the color-magnitude diagrams (CMDs) of 17 OCs using a tool called Powerful CMD, with the aim of studying the effect of inclusion of binary stars on the fitting of cluster CMDs with clear giant branches. The fitti…

2025 New Astronomy
Gaia 0
Tidal tails of nearby open clusters: I. Mapping with Gaia DR3
DOI: 10.1051/0004-6361/202453302 Bibcode: 2025A&A...694A.258R

Risbud, Dhanraj; Jadhav, Vikrant V.; Kroupa, Pavel

Context. Tidal tails of open clusters are the result of stellar evaporation from the cluster through the Galactic potential and internal dynamics. With the recent availability of high-precision data, tidal tails are being detected for most of the nearby open clusters. Aims. We identify the tidal tail members for all open clusters within a distance…

2025 Astronomy and Astrophysics
Gaia 0
The Orbits of Uranus, Its Satellites and Rings, the Gravity Field of the Uranian System, and the Orientation of the Poles of Uranus and Its Satellites
DOI: 10.3847/1538-3881/ad99d1 Bibcode: 2025AJ....169...65J

Jacobson, Robert A.; Park, Ryan S.

R. A. Jacobson determined the orbits of the Uranian satellites, the masses of Uranus and its satellites, and the orientation of the pole of Uranus from Earth-based astrometry, Earth-based ring occultations, and observations acquired with the Voyager 2 spacecraft. Subsequent to that publication, several observers obtained new astrometry, and some o…

2025 The Astronomical Journal
Gaia 0
Characterizing Stellar and Gas Properties in NGC 628: Spatial Distributions, Radial Gradients, and Resolved Scaling Relations
DOI: 10.3847/1538-4357/ad9a51 Bibcode: 2025ApJ...978..166W

Kong, Xu; Esamdin, Ali; Zou, Hu +8 more

Building on our previous research involving multiwavelength data from UV to IR, we employ spectroscopic observations of ionized gas, as well as neutral hydrogen gas obtained from the Five-hundred Meter Aperture Spherical Telescope (FAST), to explore the intrinsic processes of star formation and chemical enrichment within NGC 628. Our analysis focu…

2025 The Astrophysical Journal
XMM-Newton 0
COSMIC-S: A Photometric Catalog of Observed Stars in the Small Magellanic Cloud
DOI: 10.3847/1538-4365/adb62a Bibcode: 2025ApJS..277...33F

Franco, Antonio; Nucita, Achille A.; De Paolis, Francesco +1 more

The Dark Energy Camera (DECam) is a wide-field instrument mounted on the 4 m V. Blanco Telescope (Cerro Tololo Inter-American Observatory). Its impressive technical characteristics make it one of the most suitable ground-based telescopes for the production of accurate stellar photometry, even toward crowded regions such as the Magellanic Clouds. W…

2025 The Astrophysical Journal Supplement Series
Gaia 0