We present theoretical infrared images for Be star disks as projected on the plane of the sky. These images span a range of Be star spectral types and a wide range of disk properties and viewing inclinations. We extract the sizes of these disks at different IR wavelengths. As a test of these images, we compare our calculated disk sizes with available interferometric observations of the Be stars α Ara and ζ Tau. We use our calculated disk sizes and the observations to constrain the disk parameters of these stars
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We present a general scheme for determining the circumstellar geometry of Be stars from modeling of ...
Herbig Ae/Be objects are pre-main sequence stars surrounded by gas- and dust-rich circumstellar disc...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
International audienceContext. Be stars are rapid rotators surrounded by a gaseous disk envelope who...
We present numerical models of the circumstellar disks of Be stars, and we describe the resulting sy...
Context. The origin of the disks around Be stars is still not known. Further progress requires a pr...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
We have computed theoretical models of circumstellar disks for the classical Be stars Dra, Psc, a...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
Context. It is already accepted that Be stars are surrounded by circumstellar envelopes, which are m...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
We report theoretical HI visible and near-IR line profiles, i.e. H\( \alpha \) (6562 Å), H\( \beta ...
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We present a general scheme for determining the circumstellar geometry of Be stars from modeling of ...
Herbig Ae/Be objects are pre-main sequence stars surrounded by gas- and dust-rich circumstellar disc...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
International audienceContext. Be stars are rapid rotators surrounded by a gaseous disk envelope who...
We present numerical models of the circumstellar disks of Be stars, and we describe the resulting sy...
Context. The origin of the disks around Be stars is still not known. Further progress requires a pr...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
We have computed theoretical models of circumstellar disks for the classical Be stars Dra, Psc, a...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
Context. It is already accepted that Be stars are surrounded by circumstellar envelopes, which are m...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
We report theoretical HI visible and near-IR line profiles, i.e. H\( \alpha \) (6562 Å), H\( \beta ...
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We present a general scheme for determining the circumstellar geometry of Be stars from modeling of ...
Herbig Ae/Be objects are pre-main sequence stars surrounded by gas- and dust-rich circumstellar disc...