Showing 21–40 of 197 results
/ Date/ Name
May 1, 2020Extrapolation of Three-dimensional Magnetic Field Structure in Flare-productive Active Regions with Different Initial ConditionsMar 13, 2020Ionized outflows in local luminous AGN: what are the real densities and outflow rates?Jul 2, 2021Constraining particle acceleration in Sgr A* with simultaneous GRAVITY, Spitzer, NuSTAR and Chandra observationsSep 21, 2021The GRAVITY Young Stellar Object survey VIII. Gas and dust faint inner rings in the hybrid disk of HD141569Jan 30, 2021The GRAVITY young stellar object survey V. The orbit of the T Tauri binary star WW ChaAug 25, 20111D Modeling for Temperature-Dependent Upflow in the Dimming Region Observed by Hinode/EISMay 2, 2003Spin Susceptibility and Superexchange Interaction in the Antiferromagnet CuOSep 13, 2007Strategy for the inversion of Hinode spectropolarimetric measurements in the quiet SunNov 26, 2007Flare Ribbons Observed with G-band and FeI 6302A Filters of the Solar Optical Telescope on Board HinodeFeb 13, 2008Transient horizontal magnetic fields in solar plage regionsJun 24, 2024GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWSTMay 30, 2024High-energy neutrinos from the vicinity of the supermassive black hole in NGC 1068Dec 21, 2009Initial Results of New Tomographic Imaging of the Gamma-Ray Sky with BATSESep 24, 2025Constraints on the Orbit of the Young Substellar Companion GQ Lup B from High-Resolution Spectroscopy and VLTI/GRAVITY AstrometryAug 4, 2017Chromospheric polarimetry through multi-line observations of the 850 nm spectral region II: A magnetic flux tube scenarioApr 5, 2023The Enhanced Resolution Imager and Spectrograph for the VLTAug 29, 2025Critical photoinduced reflectivity relaxation dynamics in single-layer Bi-based cuprates near the pseudogap end pointOct 25, 2025Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034Jul 21, 2023Polarimetry and Astrometry of NIR Flares as Event Horizon Scale, Dynamical Probes for the Mass of Sgr A*Jun 29, 2023Using the motion of S2 to constrain scalar clouds around SgrA*