Showing 1–20 of 20 results
/ Date/ Name
Sep 19, 2024First Resolution of Microlensed Images of a Binary-Lens EventFeb 6, 2023Multiplicity of northern bright O-type stars with optical long baseline interferometryJan 19, 2023The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTIJun 2, 2021Progress on the calibration of surface brightness-color relations for early- and late-type starsAug 19, 2019Scalar field effects on the orbit of S2 starNov 30, 2018The Collimated Radiation in SS 433. Constraints from Spatially Resolved Optical Jets and $\texttt{Cloudy}$ Modeling of the Optical BulletsNov 30, 2018Super-Keplerian Equatorial Outflows in SS 433. Centrifugal Ejection of the Circumbinary DiskOct 17, 2018Perspectives of a visible instrument on the VLTISep 27, 2018Multiple Star Systems in the Orion NebulaSep 14, 2017The peculiar fast-rotating star 51 Oph probed by VEGA/CHARAAug 17, 2016The metrology system of the VLTI instrument GRAVITYNov 10, 2015Radii, masses, and ages of 18 bright stars using interferometry and new estimations of exoplanetary parametersJul 12, 2012The GRAVITY Coudé Infrared Adaptive Optics (CIAO) system for the VLT InterferometerJun 9, 2011The binary Be star δ Sco at high spectral and spatial resolution: Disk geometry and kinematics before the 2011 periastronJul 30, 2010First results from VLTI near-infrared interferometry on high-mass young stellar objectsNov 19, 2008The case for optical interferometric polarimetryJul 29, 2008delta Cen: a new binary Be star detected by VLTI/AMBER spectro-interferometryAug 1, 2005Planar Integrated Optics and astronomical interferometryJul 25, 2005VITRUV - Science CasesJul 10, 2005VITRUV - Imaging close environments of stars and galaxies with the VLTI at milli-arcsec resolution