Showing 41–60 of 2,286 results
/ Date/ Name
Jan 21, 2026Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branchJan 20, 2026Spectral Variability of the Star HD 141569AJan 20, 2026HD 26172: an active solar-type subgiant in a close binary systemJan 15, 2026A Highly Magnetic Ultra Massive White Dwarf with a 23-minute Rotation PeriodJan 14, 2026The Structure and Kinematics of Three Class 0 Protostellar Jets from JWSTJan 14, 2026The Progenitor of the Type II-Plateau SN 2025pht in NGC 1637: The Dustiest, Most Luminous Red Supergiant So Far?Jan 13, 2026Anatomy of Empirical Transit Spectra of Mars based on TGO/NOMADJan 9, 2026Distinct Rotational Evolution of Giant Planets and Brown Dwarf CompanionsJan 8, 2026Paving the Road to the Habitable Worlds Observatory with High-Resolution Imaging I: New and Archival Speckle Observations of Potential HWO Target StarsJan 7, 2026Predicting dust temperature from molecular line data using machine learningJan 5, 2026A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematicsJan 5, 2026Emergent Complexity in Nuclear Reaction Networks: A Study of Stellar Nucleosynthesis through Chemical Organization TheoryDec 30, 2025Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decadeDec 24, 2025The polar IL Leo in a low accretion stateDec 23, 2025Alfvénic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigationDec 18, 2025SNR 1987A : Spitzer data from days 6000 to 8000 revisitedDec 17, 2025IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emissionDec 17, 2025XRISM view of a stellar flare: High-resolution Fe K spectra of HR 1099, an RS CVn-type starDec 16, 2025The quest for Magrathea planets. II. Orbital stability of exoplanets formed around double white dwarfsDec 16, 2025Formation of a Magnetic Flux Rope Prior to the Eruption: Insight from a Radiative MHD Simulation of Active Region Emergence