Add to ORKGWe report results from mode identifications (MI) for four selected multi-periodic Slowly Pulsating B-stars (SPB) using the Fourier parameter fit (FPF) method. Problems related to the pulsational nature of these objects which hamper a correct identification are discussed. For a present day status of knowledge about SPB stars we refer to De Cat (2007, this issue)
We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsa...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
Contains fulltext : 34487.pdf ( ) (Open Access)We report results from mode identif...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
In this paper, we give an updated overview of the observed characteristics of g-mode pulsations in s...
We present the results of the mode identification for a sample of 7 bright southern slowly pulsating...
We present recent results from mode identification based on the amplitude-wavelength behaviour for t...
We present the results of the mode identification for a sample of 7 bright southern slowly pulsating...
We present recent results from mode identification based on the amplitude-wavelength behaviour for t...
We investigate the potential of multi-colour photometry for partial mode identification in both long...
In previous attempts to perform seismic modelling of pulsating subdwarf-B stars, various mode identi...
We present our results of a mode identification in several pulsating subdwarf B (sdB) stars observed...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsa...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
Contains fulltext : 34487.pdf ( ) (Open Access)We report results from mode identif...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show n...
In this paper, we give an updated overview of the observed characteristics of g-mode pulsations in s...
We present the results of the mode identification for a sample of 7 bright southern slowly pulsating...
We present recent results from mode identification based on the amplitude-wavelength behaviour for t...
We present the results of the mode identification for a sample of 7 bright southern slowly pulsating...
We present recent results from mode identification based on the amplitude-wavelength behaviour for t...
We investigate the potential of multi-colour photometry for partial mode identification in both long...
In previous attempts to perform seismic modelling of pulsating subdwarf-B stars, various mode identi...
We present our results of a mode identification in several pulsating subdwarf B (sdB) stars observed...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsa...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B...