While it is well known that most massive stars are found to be part of binary or multiple systems, an accurate characterization of the statistical properties of these multiple objects is still lacking. In the present talk, we will review the current status of the field, emphasizing the need of using complementarity techniques to cover the large parameter space. We will also describe what we think is the place of interferometry in this context.3 pages, 3 figures, to appears in the conference proceedings "The interferometric view of hot stars (2009)"status: publishe
Abstract. We report about an ongoing photometric and spectroscopic monitoring sur-vey of about 250 O...
The advent of multi-object spectrographs on 8-10 m class telescopes has provided the opportunity to ...
(Sub-)mm interferometry is the most favorable technique to investigate the earliest stages of massiv...
While it is well known that most massive stars are found to be part of binary or multiple systems, a...
While it is well known that most massive stars are found to be part of binary or multiple systems, a...
Massive binaries are crucial laboratories that allow us to investigate processes occurring in quite ...
International audienceWith the advent of large-collecting-area instruments, the number of objects th...
Abstract. Binaries are excellent astrophysical laboratories that provide us with direct measure-ment...
peer reviewedThe multiwavelength study of massive stars has revealed many phenomena that are intimat...
Observations of spectroscopic double stars with long baseline optical interferometry have resolved m...
Most main sequence massive stars (~70%) belong to short-period binaries, a fact that does not reflec...
Massive stars are characterized by a high degree of multiplicity. I will review the results of recen...
Recent advances in the development of interferometric instruments coupled to long baseline facilitie...
peer reviewedThe investigation of the multiplicity of massive stars constitutes a key aspect of thei...
Here I review the current state of the field of optical stellar interferometry, concentrating on gro...
Abstract. We report about an ongoing photometric and spectroscopic monitoring sur-vey of about 250 O...
The advent of multi-object spectrographs on 8-10 m class telescopes has provided the opportunity to ...
(Sub-)mm interferometry is the most favorable technique to investigate the earliest stages of massiv...
While it is well known that most massive stars are found to be part of binary or multiple systems, a...
While it is well known that most massive stars are found to be part of binary or multiple systems, a...
Massive binaries are crucial laboratories that allow us to investigate processes occurring in quite ...
International audienceWith the advent of large-collecting-area instruments, the number of objects th...
Abstract. Binaries are excellent astrophysical laboratories that provide us with direct measure-ment...
peer reviewedThe multiwavelength study of massive stars has revealed many phenomena that are intimat...
Observations of spectroscopic double stars with long baseline optical interferometry have resolved m...
Most main sequence massive stars (~70%) belong to short-period binaries, a fact that does not reflec...
Massive stars are characterized by a high degree of multiplicity. I will review the results of recen...
Recent advances in the development of interferometric instruments coupled to long baseline facilitie...
peer reviewedThe investigation of the multiplicity of massive stars constitutes a key aspect of thei...
Here I review the current state of the field of optical stellar interferometry, concentrating on gro...
Abstract. We report about an ongoing photometric and spectroscopic monitoring sur-vey of about 250 O...
The advent of multi-object spectrographs on 8-10 m class telescopes has provided the opportunity to ...
(Sub-)mm interferometry is the most favorable technique to investigate the earliest stages of massiv...