Reality and the speckle imaging of stellar surfaces - II. The asymmetry of Alpha Orionis

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

23

Methods: Statistical, Techniques: Interferometric, Stars: Individual: Alpha Ori, Supergiants.

Scientific paper

Bispectrum image reconstructions of the red supergiant Alpha Orionis, based upon CCD observations made with the 4.2-m William Herschel Telescope in 1995 January, are presented, and the statistical significance of asymmetries across the stellar disc established at better than 99 per cent certainty. Asymmetry is present in at least two wavebands, although the statistical evidence is stronger in the continuum than within a TiO absorption band. The asymmetry may be interpreted as being due to the presence of a bright feature contributing some 15-20 per cent of the total observed disc brightness. Ambiguities present in simple limb-darkened model fits to the power spectrum are shown, and the allowed range of limb-darkening coefficients and disc diameters is given.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Reality and the speckle imaging of stellar surfaces - II. The asymmetry of Alpha Orionis does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Reality and the speckle imaging of stellar surfaces - II. The asymmetry of Alpha Orionis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reality and the speckle imaging of stellar surfaces - II. The asymmetry of Alpha Orionis will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1810288

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.