Abstract. The orbital period is a measure of the size of a contact binary star, and can be combined with color to predict its luminosity to a fraction of stellar magnitude. This novel application of contact binary systems currently has limitations that we describe in the text but is potentially capable of providing a reasonable means of estimating distances to stellar systems at the level comparable to that achievable for Cepheids or other pulsating stars. 1
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
The mass of a star determines how it evolves throughout its lifetime from beginning to end. Understa...
Periodic variable stars, such as Cepheids, RR Lyrae, eclipsing binaries, and long-period variables, ...
The orbital period is a measure of the size of a contact binary star and can be combined with color ...
Starspots are not well understood for contact binary star systems. The following properties of spots...
V2477 Cyg is a short-period eclipsing binary star system in the Cygnus constellation. Its light curv...
New eight times of minimum light of the near-contact binary EG Cep were presented. All times of mini...
We have compiled a catalogue of light curve solutions of contact binary stars. It contains the r...
Abstract. A catalogue of 361 galactic contact binaries is presented. Listed contact binaries are div...
Periodic luminous pulses are very important for measurements in Cosmology and Astrophysics, and ther...
Cepheid variable stars have been used as “standard candles” to find distances to other stars. The fl...
This paper presents the results of a combined spectroscopic and photometric study of 20 contact bina...
We present a detailed study of the close eclipsing binary BS Vulpeculae. Although it is relatively b...
Cepheids are a class of variable (pulsating) stars whose absolute luminosities are related in a simp...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
The mass of a star determines how it evolves throughout its lifetime from beginning to end. Understa...
Periodic variable stars, such as Cepheids, RR Lyrae, eclipsing binaries, and long-period variables, ...
The orbital period is a measure of the size of a contact binary star and can be combined with color ...
Starspots are not well understood for contact binary star systems. The following properties of spots...
V2477 Cyg is a short-period eclipsing binary star system in the Cygnus constellation. Its light curv...
New eight times of minimum light of the near-contact binary EG Cep were presented. All times of mini...
We have compiled a catalogue of light curve solutions of contact binary stars. It contains the r...
Abstract. A catalogue of 361 galactic contact binaries is presented. Listed contact binaries are div...
Periodic luminous pulses are very important for measurements in Cosmology and Astrophysics, and ther...
Cepheid variable stars have been used as “standard candles” to find distances to other stars. The fl...
This paper presents the results of a combined spectroscopic and photometric study of 20 contact bina...
We present a detailed study of the close eclipsing binary BS Vulpeculae. Although it is relatively b...
Cepheids are a class of variable (pulsating) stars whose absolute luminosities are related in a simp...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
The mass of a star determines how it evolves throughout its lifetime from beginning to end. Understa...
Periodic variable stars, such as Cepheids, RR Lyrae, eclipsing binaries, and long-period variables, ...