Add to ORKGThe pre- versus post-main sequence evolutionary phase of B[e] stars Constraints from 13CO band emissio
A sample of 97 galactic field Be stars were studied by taking into account the effects induced by th...
Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100...
Aims. Not all stars exhibiting the optical spectral characteristics of B[e] stars are in the same ev...
Context. Many galactic B[e] stars suffer from improper distance determinations, which make it diffi...
We report on the first detection of 13C enhancement in two B[e] supergiants (B[e]SGs) in the Large M...
Massive evolved stars in transition phases, such as Luminous Blue Variables (LBVs), B[e] Supergiant...
Evolutionary tracks are of key importance for the understanding of star formation. Unfortunately, tr...
The evolutionary phase of B[e] stars is difficult to establish due to the uncertainties in their fun...
Massive evolved stars in transition phases, such as luminous blue variables (LBVs), B[e] supergiants...
The predicted width of the upper main sequence in stellar evolution models depends on the ...
The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on...
Contains fulltext : 72342.pdf (publisher's version ) (Closed access)We present con...
Abstract. A review on the knowledge of the stellar evolution toward the main sequence is presented. ...
Massive evolved stars in transition phases, such as luminous blue variables (LBVs), B[e] supergiants...
A sample of 97 galactic field Be stars were studied by taking into account the effects induced by th...
A sample of 97 galactic field Be stars were studied by taking into account the effects induced by th...
Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100...
Aims. Not all stars exhibiting the optical spectral characteristics of B[e] stars are in the same ev...
Context. Many galactic B[e] stars suffer from improper distance determinations, which make it diffi...
We report on the first detection of 13C enhancement in two B[e] supergiants (B[e]SGs) in the Large M...
Massive evolved stars in transition phases, such as Luminous Blue Variables (LBVs), B[e] Supergiant...
Evolutionary tracks are of key importance for the understanding of star formation. Unfortunately, tr...
The evolutionary phase of B[e] stars is difficult to establish due to the uncertainties in their fun...
Massive evolved stars in transition phases, such as luminous blue variables (LBVs), B[e] supergiants...
The predicted width of the upper main sequence in stellar evolution models depends on the ...
The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on...
Contains fulltext : 72342.pdf (publisher's version ) (Closed access)We present con...
Abstract. A review on the knowledge of the stellar evolution toward the main sequence is presented. ...
Massive evolved stars in transition phases, such as luminous blue variables (LBVs), B[e] supergiants...
A sample of 97 galactic field Be stars were studied by taking into account the effects induced by th...
A sample of 97 galactic field Be stars were studied by taking into account the effects induced by th...
Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100...
Aims. Not all stars exhibiting the optical spectral characteristics of B[e] stars are in the same ev...