In this contribution we introduce the topic of this workshop with a brief history of studies of objects with the B[e] phenomenon, including its discovery and evolution of our understanding of the phenomenon. We will also review the most prominent results on selected objects published prior to the previous B[e] star conference in 2005. These include the discovery of B[e] supergiants in the Magellanic Clouds, detection of maser and laser lines in the spectrum of MWC 349A, studies of η Carinae, and a few more. This talk is planned to set up the stage for discussion of more recent results that will be presented at the conference
B[e] supergiants (B[e]SGs) are transitional objects in the post-main sequence evolution of massive s...
We present both optical high-resolution spectroscopic and photometric observations of the FS CMa typ...
Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we hav...
Discovered over 30 years ago, the B[e] phenomenon has not yet revealed all its puzzles. New objects ...
The B[e] phenomenon was defined in the early days of infrared astronomy as a combination of the foll...
Q1 The B[e] phenomenon is defined as the simultaneous presence of low-excitation forbidden line emis...
Aims: The study is aimed at discovering new objects with the B[e] phenomenon in the Large Magellanic...
B[e] stars are massive B type emission line stars in different evolutionary stages ranging from pre-...
In this review I describe the intermediate mass pre-main-sequence Herbig Ae/Be stars and their role ...
The B[e] phenomenon is defined as the simultaneous presence of low-excitation forbidden line emissio...
This paper describes recent studies of the FS CMa-type objects, a group of stars showing the B[e] ph...
B[e] stars are massive B type emission line stars in different evolutionary stages ranging from pre-...
Aims. The study is aimed at discovering new objects with the B[e] phenomenon in the Large Magellanic...
FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emis...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
B[e] supergiants (B[e]SGs) are transitional objects in the post-main sequence evolution of massive s...
We present both optical high-resolution spectroscopic and photometric observations of the FS CMa typ...
Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we hav...
Discovered over 30 years ago, the B[e] phenomenon has not yet revealed all its puzzles. New objects ...
The B[e] phenomenon was defined in the early days of infrared astronomy as a combination of the foll...
Q1 The B[e] phenomenon is defined as the simultaneous presence of low-excitation forbidden line emis...
Aims: The study is aimed at discovering new objects with the B[e] phenomenon in the Large Magellanic...
B[e] stars are massive B type emission line stars in different evolutionary stages ranging from pre-...
In this review I describe the intermediate mass pre-main-sequence Herbig Ae/Be stars and their role ...
The B[e] phenomenon is defined as the simultaneous presence of low-excitation forbidden line emissio...
This paper describes recent studies of the FS CMa-type objects, a group of stars showing the B[e] ph...
B[e] stars are massive B type emission line stars in different evolutionary stages ranging from pre-...
Aims. The study is aimed at discovering new objects with the B[e] phenomenon in the Large Magellanic...
FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emis...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
B[e] supergiants (B[e]SGs) are transitional objects in the post-main sequence evolution of massive s...
We present both optical high-resolution spectroscopic and photometric observations of the FS CMa typ...
Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we hav...