Showing 361–380 of 2,286 results
/ Date/ Name
Apr 18, 2024VELOcities of CEpheids (VELOCE) I. High-precision radial velocities of CepheidsApr 16, 2024Maser Flares Driven by Isothermal Shock WavesApr 16, 2024Dependence of Spicule Properties on the Magnetic Field -- Results from Magnetohydrodynamics SimulationsApr 16, 2024Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometryApr 16, 2024In-depth analysis of solar models with high-metallicity abundances and updated opacity tablesApr 15, 2024Deep JWST/NIRCam imaging of Supernova 1987AApr 12, 2024Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution modelsApr 12, 2024Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovaeApr 11, 2024X-ray imaging and electron temperature evolution in laser-driven magnetic reconnection experiments at the National Ignition FacilityApr 11, 2024Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System Using High-Resolution Spectroscopy Confirms That The Companion is a Low-Mass StarApr 11, 2024Orbital dynamics in the GG Tau A system: investigating its enigmatic discApr 9, 2024OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effectsApr 2, 2024Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)Mar 29, 2024Discovery of the Longest-Period Classical Cepheid in the Milky WayMar 27, 2024Magnetic helicity evolution during active region emergence and subsequent flare productivityMar 26, 2024Alfvén Waves at MarsMar 23, 2024The First High-Contrast Images of Near High-Mass X-Ray Binaries with Keck/NIRC2Mar 22, 2024A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population propertiesMar 21, 2024Hubble Space Telescope images of SN 1987A: Evolution of the ejecta and the equatorial ring from 2009 to 2022Mar 20, 2024Application of hydrostatic local thermodynamic equilibrium atmosphere models to interpretations of supersoft X-ray source spectra