Showing 581–600 of 2,286 results
/ Date/ Name
Jan 6, 2023What does a typical full-disc around a post-AGB binary look like? -- Radiative transfer models reproducing PIONIER, GRAVITY, and MATISSE dataJan 6, 2023The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass starJan 6, 2023New insights on the near-infrared veiling of young stars using CFHT/SPIRou dataJan 5, 2023The Co-Ordinated Radio and Infrared Survey for High-Mass Star Formation. V. The CORNISH-South Survey and CatalogueJan 3, 2023Herbig Stars: A Quarter Century of ProgressDec 27, 2022Deep Learning for Space Weather Prediction: Bridging the Gap between Heliophysics Data and TheoryDec 26, 2022Population of X-ray Sources in the Intermediate-Age Cluster NGC 3532: a Test Bed for Machine-Learning ClassificationDec 23, 2022On accretion in the eclipsing polar BS TriDec 23, 2022SRGe2149+6736 -- the new candidate to AM~Her type variables discovered by eROSITA telescope on "Spectrum--Roentgen--Gamma" orbital observatoryDec 21, 2022WOCS 4540: Detailed Analysis of a Very Long Orbital Period Blue StragglerDec 19, 2022The VISCACHA survey -- VI. Dimensional study of the structure of 82 star clusters in the Magellanic CloudsDec 14, 2022New Short-Period Delta Scuti Stars in OGLE-IV Fields toward the Galactic BulgeDec 13, 2022Hyperion: The origin of the stars A far-UV space telescope for high-resolution spectroscopy over wide fieldsDec 7, 2022The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementationDec 7, 2022Gas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundanceDec 6, 2022Low Mass X-ray Binary Simulation Data ReleaseDec 5, 2022The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 FilamentNov 30, 2022Gaia Data Release 3: All-sky classification of 12.4 million variable sources into 25 classesNov 29, 2022Geomagnetic storm forecasting from solar coronal holesNov 28, 2022Revisiting Empirical Solar Energetic Particle Scaling Relations I. Solar flares