25 citations · 57 across the 6 of their papers we have counts for
6 papers
Quick Ultra-VIolet Kilonova surveyor (QUVIK)
N. Werner, J. Řípa, F. Münz +36
We present a near-UV space telescope on a ~70kg micro-satellite with a moderately fast repointing capability and a near real-time alert communication system that has been proposed…
V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?
P. Harmanec, H. Božić, P. Koubský +21
A reliable determination of the basic physical properties and variability patterns of hot emission-line stars is important for understanding the Be phenomenon and ultimately, the e…
Spectroscopy of the massive interacting binary UU Cassiopeiae
P. Hadrava, M. Cabezas, G. Djurašević +9
Context. The eclipsing close binary UU Cas is an interacting massive double-periodic system with a gainer star partly hidden in an accretion disk. Aims. In order to study the physi…
Properties and nature of Be stars 31. The binary nature, light variability, physical elements, and emission-line changes of HD~81357
P. Koubský, P. Harmanec, M. Brož +10
Reliable determination of the basic physical properties of hot emission-line binaries with Roche-lobe filling secondaries is important for developing the theory of mass exchange in…
Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138
T. Jeřábková, D. Korčáková, A. Miroshnichenko +8
We analyse spectroscopic observations of the B[e] star HD 50138 (MWC 158, V743 Mon, or IRAS 06491-0654), a member of the FS CMa group, obtained over the last twenty years. Four dif…
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 binaries
P. Harmanec, P. Koubský, J. A. Nemravová +13
Reliable determination of the basic physical properties of hot emission-line binaries with Roche-lobe filling secondaries is important for developing the theory of mass exchange in…