We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low resolution modes) and photometrically (so far 450 BVRCRIC measurements have been collected). The outburst is photometrically reminiscent of the major event BF Cyg experienced in 1890 when it rose by 4 mag in the blue. In this contribution we present the data and describe the plans to investigate this object
DM Cyg, a fundamental mode RRab star, was observed in the 2007 and 2008 seasons in the framework of ...
Context. The star V426 Sge (HBHA 1704-05), originally classified as an emission-line object and a se...
The variability of V2197 Cyg (NSVS 5761314, TYC 3167-1279-1), amongst many others, was discovered ph...
BF Cygni is a classical symbiotic binary. Its optical light curve occasionally shows outbursts of th...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
Aims. We present new results from optical photometric and spectroscopic observations of the eruptive...
We present the historical 1890-1996 photographiclB-band light curve of the symbiotic binary BF Cyg f...
New spectroscopic and photometric observations of SS Cygni, the brightest dwarf nova system, have be...
A photometric and spectral study of the variable star V2494 Cyg in the L 1003 dark cloud is presente...
Aims. Young double star V1318 Cyg, which is associated with a small isolated star-forming region aro...
WOS: 000336262600025Three presumably young eclipsing binary systems in the direction of the Cygnus O...
We present Hubble Space Telescope (HST) imaging, a Very Large Array (VLA) radio map (4.74 GHz), opti...
We present a preliminary analysis of our six-year observation campaign of the B[e] stellar system V2...
We present a large set of radio observations of the luminous blue variable P Cygni. These include tw...
DM Cyg, a fundamental mode RRab star, was observed in the 2007 and 2008 seasons in the framework of ...
Context. The star V426 Sge (HBHA 1704-05), originally classified as an emission-line object and a se...
The variability of V2197 Cyg (NSVS 5761314, TYC 3167-1279-1), amongst many others, was discovered ph...
BF Cygni is a classical symbiotic binary. Its optical light curve occasionally shows outbursts of th...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
Aims. We present new results from optical photometric and spectroscopic observations of the eruptive...
We present the historical 1890-1996 photographiclB-band light curve of the symbiotic binary BF Cyg f...
New spectroscopic and photometric observations of SS Cygni, the brightest dwarf nova system, have be...
A photometric and spectral study of the variable star V2494 Cyg in the L 1003 dark cloud is presente...
Aims. Young double star V1318 Cyg, which is associated with a small isolated star-forming region aro...
WOS: 000336262600025Three presumably young eclipsing binary systems in the direction of the Cygnus O...
We present Hubble Space Telescope (HST) imaging, a Very Large Array (VLA) radio map (4.74 GHz), opti...
We present a preliminary analysis of our six-year observation campaign of the B[e] stellar system V2...
We present a large set of radio observations of the luminous blue variable P Cygni. These include tw...
DM Cyg, a fundamental mode RRab star, was observed in the 2007 and 2008 seasons in the framework of ...
Context. The star V426 Sge (HBHA 1704-05), originally classified as an emission-line object and a se...
The variability of V2197 Cyg (NSVS 5761314, TYC 3167-1279-1), amongst many others, was discovered ph...