DOIAbstract
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and luminosity classes III, IV & V. The H
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and luminosity classes III, IV & V. The H
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
This chapter describes non supergiant B-type stars that show emission lines, called Be stars. The em...
Both high and medium resolution spectroscopy of the Be stars and binary stellar systems in the young...
We present K band (2.05 μm - 2.22 μm) spectra of 66 isolated Be stars of spectral types O9-B9 and ...
Abstract. We present K band (2.05 m − 2.22 m) spec-tra of 66 isolated Be stars of spectral types O9-...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
and other research outputs A representative sample of Be stars III: H band spec-troscop
A Be star is defined as a non-supergiant B star whose spectrum, either in the past or present, conta...
Abstract. We present here the H spectra of 44 Be stars taken at a resolution of 0.5 A. From the spe...
From a survey of spectra of Bn/An stars, we have detected seven new Be stars: HR 1056 (A0Vn), 1544 (...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity cl...
International audienceBe stars vary on many timescales, from hours to decades. A long time base of o...
Context. It is already accepted that Be stars are surrounded by circumstellar envelopes, which are m...
Abstract. | A sample of 37 stars of luminosity classes I, III, V, including few SMR stars observed i...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
This chapter describes non supergiant B-type stars that show emission lines, called Be stars. The em...
Both high and medium resolution spectroscopy of the Be stars and binary stellar systems in the young...
We present K band (2.05 μm - 2.22 μm) spectra of 66 isolated Be stars of spectral types O9-B9 and ...
Abstract. We present K band (2.05 m − 2.22 m) spec-tra of 66 isolated Be stars of spectral types O9-...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
and other research outputs A representative sample of Be stars III: H band spec-troscop
A Be star is defined as a non-supergiant B star whose spectrum, either in the past or present, conta...
Abstract. We present here the H spectra of 44 Be stars taken at a resolution of 0.5 A. From the spe...
From a survey of spectra of Bn/An stars, we have detected seven new Be stars: HR 1056 (A0Vn), 1544 (...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity cl...
International audienceBe stars vary on many timescales, from hours to decades. A long time base of o...
Context. It is already accepted that Be stars are surrounded by circumstellar envelopes, which are m...
Abstract. | A sample of 37 stars of luminosity classes I, III, V, including few SMR stars observed i...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
This chapter describes non supergiant B-type stars that show emission lines, called Be stars. The em...
Both high and medium resolution spectroscopy of the Be stars and binary stellar systems in the young...
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