Showing 421–440 of 1,412 results
/ Date/ Name
Mar 1, 2023A major asymmetric ice trap in a planet-forming disk IV. Nitric oxide gas and a lack of CN tracing sublimating ices and a C/O ratio $< 1$Feb 21, 2023TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPSFeb 21, 2023The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)Feb 20, 2023Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging MissionsFeb 17, 2023Jupiter's interior from Juno: Equation-of-state uncertainties and dilute core extentFeb 16, 2023Revising Properties of Planet-Host Binary Systems. III. There is No Observed Radius Gap For Kepler Planets in Binary Star SystemsFeb 13, 2023Direct imaging discovery of a super-Jovian around the young Sun-like star AF LeporisFeb 11, 2023ALMA Band 6 high-resolution observations of the transitional disk around SY ChaFeb 9, 2023Demographics of Protoplanetary Disks: A Simulated Population of Edge-on SystemsFeb 7, 2023Precession and polar alignment of accretion discs in triple (or multiple) stellar systemsFeb 2, 2023NEOROCKS project: surface properties of small near-Earth asteroidsJan 26, 2023High Speed Focal Plane Wavefront Sensing with an Optical ChopperJan 25, 2023Early stages of Galilean moon formation in a water-depleted environmentJan 25, 2023Surveying Nearby Brown Dwarfs with HGCA: Direct Imaging Discovery of a Faint, High-Mass Brown Dwarf Orbiting HD 176535 AJan 23, 2023Mercury's formation within the Early Instability ScenarioJan 20, 2023Tidal Distortions as a Bottleneck on Constraining Exoplanet CompositionsJan 17, 2023Dynamical tides in Jupiter and other rotationally flattened planets and stars with stable stratificationJan 16, 2023A First Look at the JWST MIRI/LRS Phase Curve of WASP-43bJan 11, 2023New members of the Lupus I cloud based on Gaia astrometry Physical and accretion properties from X-Shooter spectraJan 10, 2023Detecting exomoons from radial velocity measurements of self-luminous planets: application to observations of HR 7672 B and future prospects