activity
20102022
most citedSpectroscopic survey of emission-line stars. I. B[e] stars

45 citations · 85 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022★ 5 cited

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…

astro-ph.SR2019★ 8 cited

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…

astro-ph.GA2016★ 2 cited

The orbital elements and physical properties of the eclipsing binary BD+36 3317, a probable member of Lyr cluster

E. Kıran, P. Harmanec, Ö. L. Değirmenci +4

Context. The fact that eclipsing binaries belong to a stellar group is useful, because the former can be used to estimate distance and additional properties of the latter, and vice…

astro-ph.SR2015★ 45 cited

Spectroscopic survey of emission-line stars. I. B[e] stars

Anna Aret, Michaela Kraus, Miroslav Šlechta

Emission-line stars are typically surrounded by dense circumstellar material, often in form of rings or disc-like structures. Line emission from forbidden transitions trace a diver…

astro-ph.SR2014★ 25 cited

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…

astro-ph.SR2010

A new ephemeris and an orbital solution of ε Aurigae

Pavel Chadima, Petr Harmanec, Stephenson Yang +9

We collected rich series of RV measurements covering last 110 years and photometric observations from the past 6 primary eclipses, complemented them by our new observations and der…