Showing 21–40 of 2,286 results
/ Date/ Name
Feb 27, 2026Stellar engines and Dyson bubbles can be stableFeb 27, 2026The Split Janus-faced Sun: Magnetic Rhythm and Duality in the Solar CycleFeb 24, 2026A Path to an All-Sky Survey with RomanFeb 23, 2026Long Photometric Cycles in Double Periodic Variables from Nodal Precession of a Tilted Accretion DiskFeb 17, 2026Molecular diagnostics for the mid-infrared emission of planet-forming disks. Carbon and oxygen elemental abundancesFeb 16, 2026Barium Stars Across the Milky Way: Probing Their Origins via the GALAH SurveyFeb 12, 2026Parker Solar Probe observations of solar energetic particle (SEP) events with inverse velocity arrival (IVA) featuresFeb 10, 2026Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMAFeb 10, 2026Observing solar vortices with existing and future instrumentation. Solar Physics International Network for Swirls (SPINS) white paper (Helio)Feb 9, 2026A mapping method of age estimation for binary stars: Application to the $α$ Centauri system A and BFeb 6, 2026AB Aur, a Rosetta stone for studies of planet formation (IV): C/O estimates from CS and SO interferometric observationsFeb 6, 2026The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region EmergenceFeb 6, 2026The Walkaway Star HP Tau/G2: Evidence for a Stellar MergerFeb 3, 2026The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812Feb 3, 2026A surprisingly large asymmetric ejection from Mira AFeb 3, 2026FORGE'd in the Early Universe: The Effect of Protostellar Outflows on Pop III AccretionFeb 2, 2026Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded PictureFeb 2, 2026Noble gases Neon and argon: a role for the chemical patterns of multiple populations in globular clusters?Jan 28, 202627 years of Spaceborne IR Astronomy: An ISO, Spitzer, WISE and NEOWISE Survey for Large-Amplitude Variability in Young Stellar ObjectsJan 27, 2026An analysis of the J-method from the perspective of the AGB evolution