Contains fulltext : 134834.pdf (preprint version ) (Open Access
Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous...
Aims: We present the first near-IR milli-arcsecond-scale image of a post-AGB binary that is surround...
Several classes of evolved stars contain highly luminous objects, which, more often than not, are ch...
Context. The presence of stable disks around post-asymptotic giant branch (post-AGB) binaries is a w...
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Context. The presence of stable disks around post-asymptotic giant branch (post-AGB) binaries is a w...
Abstract. Binaries with circumbinary disks are commonly found among optically bright post-AGB stars....
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Binaries with circumbinary disks are commonly found among optically bright post-AGB stars. Although ...
Several post-AGB binaries appear to be surrounded by disks of dust and gas. These disks are formed f...
Several post-AGB binaries appear to be surrounded by disks of dust and gas. These disks are formed f...
Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous...
It is now well established that FGK post-AGB stars that are surrounded by both hot and cold dust (as...
It is now well established that FGK post-AGB stars that are surrounded by both hot and cold dust (as...
Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous...
Aims: We present the first near-IR milli-arcsecond-scale image of a post-AGB binary that is surround...
Several classes of evolved stars contain highly luminous objects, which, more often than not, are ch...
Context. The presence of stable disks around post-asymptotic giant branch (post-AGB) binaries is a w...
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Context. The presence of stable disks around post-asymptotic giant branch (post-AGB) binaries is a w...
Abstract. Binaries with circumbinary disks are commonly found among optically bright post-AGB stars....
Context. Binary post-asymptotic giant branch (post-AGB) stars are interesting laboratories to study ...
Binaries with circumbinary disks are commonly found among optically bright post-AGB stars. Although ...
Several post-AGB binaries appear to be surrounded by disks of dust and gas. These disks are formed f...
Several post-AGB binaries appear to be surrounded by disks of dust and gas. These disks are formed f...
Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous...
It is now well established that FGK post-AGB stars that are surrounded by both hot and cold dust (as...
It is now well established that FGK post-AGB stars that are surrounded by both hot and cold dust (as...
Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous...
Aims: We present the first near-IR milli-arcsecond-scale image of a post-AGB binary that is surround...
Several classes of evolved stars contain highly luminous objects, which, more often than not, are ch...
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