We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity classes III to V. We have obtained 3670 – 5070 Å spectra of the sample which are used to derive spectral types and rotational velocities. We discuss the distribution of spectral types and rotational velocities obtained and conclude that there are no significant selection effects in our sample
We present an atlas of Hγ, He i λ 4471 and Mg ii λ 4481 line profiles obtained in a 10 year observat...
Be stars are B-type main-sequence stars that display broad Balmer emission lines in their spectra. I...
25 pages, 9 figures, Accepted for publication in A&AIn preparation for the COROT space mission, we d...
We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity cl...
and other research outputs A representative sample of Be Stars I: sample selection, spectral classif...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III,...
Abstract. We present K band (2.05 m − 2.22 m) spec-tra of 66 isolated Be stars of spectral types O9-...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Spectroscopic monitoring of 141 southern field B type stars, 114 of them known to exhibit the ...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
International audienceWe present an atlas of Hγ , He i lambda 4471 and Mg ii lambda 4481 line profil...
Massive O- and B-type stars are cosmic engines in the Universe and can be the dominant source of l...
We present an atlas of Hγ, He i λ 4471 and Mg ii λ 4481 line profiles obtained in a 10 year observat...
Be stars are B-type main-sequence stars that display broad Balmer emission lines in their spectra. I...
25 pages, 9 figures, Accepted for publication in A&AIn preparation for the COROT space mission, we d...
We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity cl...
and other research outputs A representative sample of Be Stars I: sample selection, spectral classif...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III,...
Abstract. We present K band (2.05 m − 2.22 m) spec-tra of 66 isolated Be stars of spectral types O9-...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Spectroscopic monitoring of 141 southern field B type stars, 114 of them known to exhibit the ...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
International audienceWe present an atlas of Hγ , He i lambda 4471 and Mg ii lambda 4481 line profil...
Massive O- and B-type stars are cosmic engines in the Universe and can be the dominant source of l...
We present an atlas of Hγ, He i λ 4471 and Mg ii λ 4481 line profiles obtained in a 10 year observat...
Be stars are B-type main-sequence stars that display broad Balmer emission lines in their spectra. I...
25 pages, 9 figures, Accepted for publication in A&AIn preparation for the COROT space mission, we d...