Reference : Prospects for the study of dust making Wolf-Rayet binaries with the VLTI-Spectro-Imag...
Scientific congresses and symposiums : Paper published in a journal
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/11561
Prospects for the study of dust making Wolf-Rayet binaries with the VLTI-Spectro-Imager (VSI)
English
De Becker, Michaël mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Sciences spatiales >]
Filho, M. [>]
Harries, T. [>]
Feb-2010
Revista Mexicana de Astronomía y Astrofísica
Universidad Nacional Autónoma de México
38
The Interferometric View on Hot Stars
59
No
No
International
0185-1101
México
The Interferometric View on Hot Stars
du 2 au 6 mars 2009
ESO
Vina del Mar
Chili
[en] Interferometry ; Massive stars ; Binaries ; Dust
[en] In response to ESO's call for proposals for second generation instruments for the Very Large Telescope Interferometer (VLTI), a consortium has proposed to design and develop the VLTI-Spectro-Imager (VSI). In the context of the Phase A study, a science group has prepared a science case taking advantage of the expected performances of VSI. Among several science topics, the case of dust making Wolf-Rayet binaries producing the so-called pinwheel nebulae has been considered. Here, we review the main specifications of VSI, and we provide preliminary results expected to illustrate the imaging capabilities of VSI, and the interest for the study of pinwheel nebulae similar to those formed close to well-known systems such as WR98a and WR104.
Researchers ; Professionals
http://hdl.handle.net/2268/11561
http://adsabs.harvard.edu/abs/2010RMxAC..38...59D

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