Showing 1–18 of 18 results
/ Date/ Name
Nov 28, 2000Properties and nature of Be stars. XX. Binary nature and orbital elements of gamma CasJan 23, 2004Properties and nature of Be stars XXIII. Long-term variations and physical properties of kappa DraSep 1, 2009Disentangling of spectra - theory and practiceMar 25, 2010Fourier Disentangling Using the Technology of Virtual ObservatoryMar 2, 2022HR 6819 is a binary system with no black hole -- revisiting the source with infrared interferometry and optical integral field spectroscopySep 18, 2009HD172189: another step in furnishing one of the best laboratories known for asteroseismic studiesSep 3, 2009Notes on disentangling of spectra II. Intrinsic line-profile variability due to Cepheid pulsationsAug 25, 2022MWC656: A Be+BH or a Be+sdO?Jul 13, 2010Spectroscopic analysis of the B/Be visual binary HR 1847Dec 12, 2024Newborn Be star systems observed shortly after mass transferSep 2, 2020New insights on the massive interacting binary UU CassiopeiaeMay 6, 2020A naked-eye triple system with a nonaccreting black hole in the inner binaryJan 31, 2022Spectroscopy of the massive interacting binary UU CassiopeiaeJul 14, 2009The Ultraviolet Spectrum and Physical Properties of the Mass Donor Star in HD 226868 = Cygnus X-1Jan 28, 2008Stellar Wind Variations During the X-ray High and Low States of Cygnus X-1May 10, 2019On the long cycle variability of the Algol OGLE-LMC-DPV-065 and its stellar, orbital and disk parametersFeb 11, 2025Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1Jan 7, 2025VLTI/GRAVITY enables the determination of the first dynamical masses of a classical Be + stripped and bloated pre-subdwarf binary