- New Findings Supporting the Presence of Several Distinct Structures of Circumstellar Matter in â Lyr?2007 | Faculty of Mathematics and Physics
- INVESTIGATING THE CIRCUMSTELLAR DISK OF THE Be SHELL STAR 48 LIBRAE2016 | Faculty of Mathematics and Physics
- A Comprehensive Analysis of Spitzer Supernovae2019 | Faculty of Mathematics and Physics
- Modeling of interactions between supernovae ejecta and aspherical circumstellar environments2019 | Faculty of Mathematics and Physics
- Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon +12013 | Faculty of Mathematics and Physics
- Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 501382016 | Faculty of Mathematics and Physics
- Supernova explosions interacting with aspherical circumstellar material: implications for light curves, spectral line profiles, and polarization2020 | Faculty of Mathematics and Physics
- Formation of NaCl by radiative association in interstellar environments2022 | Faculty of Mathematics and Physics
- PHOTODETACHMENT AS A DESTRUCTION MECHANISM FOR CN- AND C3N- ANIONS IN CIRCUMSTELLAR ENVELOPES2013 | Faculty of Mathematics and Physics
- Kinematics of mass-loss from the outer Lagrange point L22019 | Faculty of Mathematics and Physics
- Revealing the structure of the outer disks of Be stars2017 | Faculty of Mathematics and Physics
- A high angular and spectral resolution view into the hidden companion of epsilon Aurigae2012 | Faculty of Mathematics and Physics
- First detection of a magnetic field in low-luminosity B[e] stars New scenarios for the nature and evolutionary stages of FS CMa stars2022 | Faculty of Mathematics and Physics
- Spectroscopy of the massive interacting binary UU Cassiopeiae2022 | Faculty of Mathematics and Physics
- Improved estimates of the physical properties of the O-star binary V1007 Sco = HD 152248 and notes on several other binaries in the NGC 6231 cluster2008 | Faculty of Mathematics and Physics
- Properties and nature of Be stars 31. The binary nature, light variability, physical elements, and emission-line changes of HD 813572019 | Faculty of Mathematics and Physics
- Properties and nature of Be stars 30. Reliable physical properties of a semi-detached B9.5e+G8III binary BR CMi = HD 61273 compared to those of other well studied semi-detached emission-line binaries2015 | Faculty of Mathematics and Physics
- New insights on the massive interacting binary UU Cassiopeiae2020 | Faculty of Mathematics and Physics