Latest Research in Solar and Stellar Astrophysics
31 research papers · 2026 median publication year
Top Research Topics in Solar and Stellar Astrophysics
- Astrophysics of Galaxies — 9 papers
- Solar and Stellar Astrophysics — 8 papers
- Earth and Planetary Astrophysics — 5 papers
- Astrophysics and Star Formation Studies — 3 papers
- Galaxies: Formation, Evolution, Phenomena — 2 papers
- High Energy Astrophysical Phenomena — 2 papers
- Instrumentation and Methods for Astrophysics — 1 papers
- Stellar, planetary, and galactic studies — 1 papers
Highest-Cited Papers
- A useful representation of TESS light curves
- The JWST Sub-Jupiters Survey: Direct Imaging Discovery of a Giant Planet and a Debris Disk Around the Young M-dwarf RX J0534.0-0221
- The Galactic centre G+0.633-0.0604 molecular cloud: A new astrochemical gold mine: II. Chemical richness
- A homogeneous analysis of archival and new low-resolution spectra of YZ Cancri
- Interferometric Survey of Stellar Parameters: Limb darkening study with the "Pipeline for Interferometric Measurements of Stars"
- Mapping Molecular Ion Distributions in a Diverse Sample of Protoplanetary Disks
- Sub-arcsecond imaging of HCN and CN in the Orion Bar. UV-driven warm Nitrogen chemistry in dense environments
- Dust Seeding Molecules in a Massive Protostar -- Detection of TiO in Orion Source I
- Proto-Planetary Nebulae Are Not the Precursors of Planetary Nebulae With Close Binary Central Stars
- Common Excitation Patterns of Star Formation, Active Galactic Nuclei, and Shocks in Seyfert Galaxies
- Searching for Black Hole Candidates in Quiescence by Using Multi-band Observations in Globular Cluster M22 (NGC 6656)
- Exploration of groups and outliers in Gaia RVS stellar spectra with metric learning
- Recovering turbulent velocity statistics from noisy integral-field spectroscopy
- JWST/MIRI Imaging Search for Kinematically Detected Protoplanetary Candidates
- The FU Ori outburst of PR Ori B
- Predictions for astrometric microlensing in Gaia
- OPTIMus-Survey of massive star-forming regions at OPTical, Infrared, and Millimeter wavelengths
- XUE. ProDiMo models of internally and externally irradiated planet-forming disks around 0.3-4.0 solar mass stars (The IRIS project I)
- Origins of complex organic molecules in L1551 IRS 5: Interplay of thermal heating and accretion shocks
- Dust Substructures and Line Perturbations driven by a Forming Planet in J16120