International audienceOne of the most attractive events in the pre-main sequence evolution is the FU Orionis (FUor) outburst. Because only a small number of FUor stars have been detected to date, photometric and spectral studies of every new object are of great interest. Recently, a new FUor candidate was discovered by Anton Khruslov - V582 Aur. To confirm the FUors nature of this object we started regular photometric observations with the telescopes of the National Astronomical Observatory Rozhen (Bulgaria). A high-resolution spectrum of V582 Aur was obtained with the 1.93 m telescope in Haute-Provence Observatory (France)
V582 Aur is a pre-main-sequence FU Orionis type eruptive star, which entered a brightness minimum in...
Aims. We present new results from optical photometric and spectroscopic observations of the eruptive...
We present Herschel-HIFI, SPIRE, and PACS 50-670 mu m imaging and spectroscopy of six FU Orionis-typ...
International audience Aims: We present results from optical photometric and spectroscopic observati...
For several decades we have been performing photometric monitoring of some of the star formation reg...
We present results from photometric monitoring of V900 Mon, one of the newly discovered and still...
The early evolution of Sun-like stars may be interspersed by energetic FU Orionis (FUor) type accret...
V582 Aur is an FU Ori-type young eruptive star in outburst since ̃1985. The eruption is currently in...
Results from optical photometric observations of the PMS star V 1735 Cyg are reported. On the basis ...
Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are...
ArticleDuring their formation phase stars gain most of their mass in violent episodic accretion even...
The earliest phases of star formation are characterised by intense mass accretion from the circumste...
V582 Aur is a pre-main-sequence FU Orionis type eruptive star, which entered a brightness minimum in...
By using the Adaptive Optics with a Laser for Astronomy system at the 3.6 m telescope of the Ca...
Context. The FU Orionis candidate V733 Cep was discovered by Roger Persson in 2004. The star is lo...
V582 Aur is a pre-main-sequence FU Orionis type eruptive star, which entered a brightness minimum in...
Aims. We present new results from optical photometric and spectroscopic observations of the eruptive...
We present Herschel-HIFI, SPIRE, and PACS 50-670 mu m imaging and spectroscopy of six FU Orionis-typ...
International audience Aims: We present results from optical photometric and spectroscopic observati...
For several decades we have been performing photometric monitoring of some of the star formation reg...
We present results from photometric monitoring of V900 Mon, one of the newly discovered and still...
The early evolution of Sun-like stars may be interspersed by energetic FU Orionis (FUor) type accret...
V582 Aur is an FU Ori-type young eruptive star in outburst since ̃1985. The eruption is currently in...
Results from optical photometric observations of the PMS star V 1735 Cyg are reported. On the basis ...
Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are...
ArticleDuring their formation phase stars gain most of their mass in violent episodic accretion even...
The earliest phases of star formation are characterised by intense mass accretion from the circumste...
V582 Aur is a pre-main-sequence FU Orionis type eruptive star, which entered a brightness minimum in...
By using the Adaptive Optics with a Laser for Astronomy system at the 3.6 m telescope of the Ca...
Context. The FU Orionis candidate V733 Cep was discovered by Roger Persson in 2004. The star is lo...
V582 Aur is a pre-main-sequence FU Orionis type eruptive star, which entered a brightness minimum in...
Aims. We present new results from optical photometric and spectroscopic observations of the eruptive...
We present Herschel-HIFI, SPIRE, and PACS 50-670 mu m imaging and spectroscopy of six FU Orionis-typ...