AbstractWe 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
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We report theoretical HI visible and near-IR line profiles, i.e. H\( \alpha \) (6562 Å), H\( \beta ...
We present theoretical infrared images for Be star disks as projected on the plane of the sky. These...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Be stars are rapidly rotating B-type stars that eject large amounts of material into a circumstellar...
We present spectrophotometric data from 0.4 μm to 4.2 μm for bright, northern sky, Be stars and seve...
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...
Through the modeling of near-infrared photometry of star-plus disk systems with the codes bedisk/ber...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
We present the first K'-band, long-baseline interferometric observations of the northern Be stars ga...
Astronomy & Astrophysics 586 (2016): A6 reproduced with permission from Astronomy & AstrophysicsHerb...
Identify physical conditions of B-emission stars at certain positions over specific wavelengths. Cla...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We report theoretical HI visible and near-IR line profiles, i.e. H\( \alpha \) (6562 Å), H\( \beta ...
We present theoretical infrared images for Be star disks as projected on the plane of the sky. These...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Be stars are rapidly rotating B-type stars that eject large amounts of material into a circumstellar...
We present spectrophotometric data from 0.4 μm to 4.2 μm for bright, northern sky, Be stars and seve...
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...
Through the modeling of near-infrared photometry of star-plus disk systems with the codes bedisk/ber...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
We present the first K'-band, long-baseline interferometric observations of the northern Be stars ga...
Astronomy & Astrophysics 586 (2016): A6 reproduced with permission from Astronomy & AstrophysicsHerb...
Identify physical conditions of B-emission stars at certain positions over specific wavelengths. Cla...
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar envel...
International audienceContext. HD 110432 was classified as a “γ Cas X-ray analog” since it has simil...
We report theoretical HI visible and near-IR line profiles, i.e. H\( \alpha \) (6562 Å), H\( \beta ...