Add to ORKGHD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic monitoring over 5 years reveals strong variations in the strength of the emission lines and for HD 45314 in the V/R ratio of the double-peaked emissions. Part of these long-term variations could be recurrent.status: publishe
We present here the results and interpretation of a long-term OH variability program conducted with...
We present and interpret the results of a long-term OH variability study of three semiregular stars...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
HD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic monitoring over 5 years reveal...
Context. The two Oe stars HD 45 314 and HD 60 848 have recently been found to exhibit very different...
We present the very first analysis of the spectroscopic variability of the three rapidly rotating Oe...
Context. Plaskett’s star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. B[e] stars are anomalous objects around which extended circumstellar matter is present. The...
Received date / Accepted date Context. Oe stars possibly form an extension to higher temperatures of...
Context. A growing number of Be and Oe stars, named the γ Cas stars, are known for their unusually h...
peer reviewedWe analyse the spectroscopic and photometric variability of the Oe star HD 60 848 over ...
Context. Plaskett’s star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. Plaskett's star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. A growing number of Be and Oe stars, named the γ Cas stars, are known for their unusually h...
The transition from early Of stars to WN-type objects is poorly understood. O-type supergiants with ...
We present here the results and interpretation of a long-term OH variability program conducted with...
We present and interpret the results of a long-term OH variability study of three semiregular stars...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
HD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic monitoring over 5 years reveal...
Context. The two Oe stars HD 45 314 and HD 60 848 have recently been found to exhibit very different...
We present the very first analysis of the spectroscopic variability of the three rapidly rotating Oe...
Context. Plaskett’s star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. B[e] stars are anomalous objects around which extended circumstellar matter is present. The...
Received date / Accepted date Context. Oe stars possibly form an extension to higher temperatures of...
Context. A growing number of Be and Oe stars, named the γ Cas stars, are known for their unusually h...
peer reviewedWe analyse the spectroscopic and photometric variability of the Oe star HD 60 848 over ...
Context. Plaskett’s star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. Plaskett's star (HD 47129) is a very massive O-star binary in a post Roche-lobe overflow st...
Context. A growing number of Be and Oe stars, named the γ Cas stars, are known for their unusually h...
The transition from early Of stars to WN-type objects is poorly understood. O-type supergiants with ...
We present here the results and interpretation of a long-term OH variability program conducted with...
We present and interpret the results of a long-term OH variability study of three semiregular stars...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...