Recently we have demonstrated that high-precision polarization observations can detect the polarization resulting from the rotational distortion of a rapidly rotating B-type star. Here, we investigate the extension of this approach to an A-type star. Linear-polarization observations of α Oph (A5IV) have been obtained over wavelengths from 400 to 750 nm. They show the wavelength dependence expected for a rapidly rotating star combined with a contribution from interstellar polarization. We model the observations by fitting rotating-star polarization models and adding additional constraints including a measured vesin i. However, we cannot fully separate the effects of rotation rate and inclination, leaving a range of possible solutions. We det...
This is the author accepted manuscript. The final version is available from the American Astronomica...
We report observations of the linear polarization of a sample of 50 nearby Southern bright stars mea...
The nearby star a Oph (Ras Alhague) is a rapidly rotating A5IV star spinning at ∼ 89% of its breakup...
Recently we have demonstrated that high-precision polarization observations can detect the polarizat...
Recently we have demonstrated that high-precision polarization observations can detect the polarizat...
Aims. The fact that the O-type close binary star system AO Cassiopeiae exhibits variable phase-locke...
International audienceWe have observed the active starξBoo A (HD 131156A) with high precision br...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing. ...
We present linear Hα spectropolarimetry of the classical T Tauri star RY Tau. A change in the polar...
Context. While there is evidence for considerable circular polarization of OH masers in star-forming...
We have observed the active star ξ Boo A (HD 131156A) with high precision broadband linear polarimet...
Aims. To detect line effects using spectropolarimetry in order to find evidence of rotating disks an...
We have designed and built a prototype imaging polarimeter for use on the PROMPT robotic telescopes ...
Classical T Tauri stars are encircled by accretion discs most of the time unresolved by conventiona...
Original paper can be found at: http://www.aspbooks.org/ Copyright ASPWe present emission line polar...
This is the author accepted manuscript. The final version is available from the American Astronomica...
We report observations of the linear polarization of a sample of 50 nearby Southern bright stars mea...
The nearby star a Oph (Ras Alhague) is a rapidly rotating A5IV star spinning at ∼ 89% of its breakup...
Recently we have demonstrated that high-precision polarization observations can detect the polarizat...
Recently we have demonstrated that high-precision polarization observations can detect the polarizat...
Aims. The fact that the O-type close binary star system AO Cassiopeiae exhibits variable phase-locke...
International audienceWe have observed the active starξBoo A (HD 131156A) with high precision br...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing. ...
We present linear Hα spectropolarimetry of the classical T Tauri star RY Tau. A change in the polar...
Context. While there is evidence for considerable circular polarization of OH masers in star-forming...
We have observed the active star ξ Boo A (HD 131156A) with high precision broadband linear polarimet...
Aims. To detect line effects using spectropolarimetry in order to find evidence of rotating disks an...
We have designed and built a prototype imaging polarimeter for use on the PROMPT robotic telescopes ...
Classical T Tauri stars are encircled by accretion discs most of the time unresolved by conventiona...
Original paper can be found at: http://www.aspbooks.org/ Copyright ASPWe present emission line polar...
This is the author accepted manuscript. The final version is available from the American Astronomica...
We report observations of the linear polarization of a sample of 50 nearby Southern bright stars mea...
The nearby star a Oph (Ras Alhague) is a rapidly rotating A5IV star spinning at ∼ 89% of its breakup...