activity
20112026
most citedPhysical properties of beta Lyr A and its opaque accretion disk

20 citations · 35 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

Interferometric Survey of Stellar Parameters: Mass of the metallic A-type binary Aur

J. Jonák, D. Mourard, J. D. Monnier +23

With the capabilities of the new visible CHARA/SPICA instrument and the multiple spectral band operation of CHARA, our goal is to resolve orbits of short-period binaries and develo…

astro-ph.SR2026

Refined reduction and standardisation of 53 years of UBV photometry at Hvar

Hrvoje Božić, Petr Harmanec, Miroslav Brož +17

Emission-line stars classified as Be exhibit light and colour variability on various timescales, ranging from days to decades. Their evolution must be constrained by long-term obse…

astro-ph.SR2026

VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr

D. Jadlovský, M. Wittkowski, A. Chiavassa +9

The mass-loss process of red supergiant (RSG) and asymptotic giant branch (AGB) stars and its relation to variability are poorly constrained. We study two evolved stars, the Mira-t…

astro-ph.SR2022★ 6 cited

Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinæ: II. N-body model

M. Brož, P. Harmanec, P. Zasche +16

HD 93206 is early-type massive stellar system, composed of components resolved by direct imaging (Ab, Ad, B, C, D) as well as a compact sub-system (Aa1, Aa2, Ac1, Ac2). Its geometr…

astro-ph.SR2022★ 3 cited

Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinae - I. Observations and their initial analyses

P. Harmanec, P. Zasche, M. Brož +17

The hot nine-component system HD 93206, which contains a gravitationally bounded eclipsing Ac1+Ac2 binary (~d) and a spectroscopic Aa1+Aa2 (~d) binary can provi…

astro-ph.SR2018★ 20 cited

Physical properties of beta Lyr A and its opaque accretion disk

D. Mourard, M. Broz, J. Nemravova +23

Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes…

astro-ph.SR2017★ 4 cited

Improved model of the triple system V746 Cas that has a bipolar magnetic field associated with the tertiary

P. Harmanec, M. Brož, P. Mayer +9

V746 Cas is known to be a triple system composed of a close binary with an alternatively reported period of either 25.4d or 27.8d and a third component in a 62000d orbit. The objec…

astro-ph.SR2011★ 2 cited

V2368 Oph: An eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Oph

P. Harmanec, H. Božić, P. Mayer +8

The A-type star HR 6412 = V2368 Oph was used by several investigators as a photometric comparison star for the known eclipsing binary U Oph but was found to be variable by three in…