Add to ORKGWe present a preliminary analysis of our five-years observation campaign of the B[e] stellar system V2028 Cyg (MWC 623). The time variability of spectral features is described
ABSTRACT Context. Massive eclipsing double lined spectroscopic binaries are not comon but are necesa...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassiv...
We present a preliminary analysis of our six-year observation campaign of the B[e] stellar system V2...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
We present results of nearly six years of spectroscopic observations of the B[e] star V2028 Cyg. The...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
This paper describes recent studies of the FS CMa-type objects, a group of stars showing the B[e] ph...
WOS: 000185676200023New photometric observations of the Algol-type binary system AB Cassiopeiae were...
B[e] supergiant stars (B[e]SGs) are a rare and unusual class of massive evolved stars which are poor...
Context. The mechanism by which supergiant (sg)B[e] stars support cool, dense dusty discs/tori and t...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
Context. The mechanism by which supergiant (sg)B[e] stars support cool, dense dusty discs/tori and t...
ABSTRACT Context. Massive eclipsing double lined spectroscopic binaries are not comon but are necesa...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassiv...
We present a preliminary analysis of our six-year observation campaign of the B[e] stellar system V2...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
We present results of nearly six years of spectroscopic observations of the B[e] star V2028 Cyg. The...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
This paper describes recent studies of the FS CMa-type objects, a group of stars showing the B[e] ph...
WOS: 000185676200023New photometric observations of the Algol-type binary system AB Cassiopeiae were...
B[e] supergiant stars (B[e]SGs) are a rare and unusual class of massive evolved stars which are poor...
Context. The mechanism by which supergiant (sg)B[e] stars support cool, dense dusty discs/tori and t...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
Context. The mechanism by which supergiant (sg)B[e] stars support cool, dense dusty discs/tori and t...
ABSTRACT Context. Massive eclipsing double lined spectroscopic binaries are not comon but are necesa...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
Context. The TeV BL Lac object PG 1553+113 is one of the primary candidates for a binary supermassiv...