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Imaging the surface of Altair.

John D Monnier1, M Zhao, E Pedretti

  • 1Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA. monnier@umich.edu

Science (New York, N.Y.)
|June 2, 2007
PubMed
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We imaged the star Altair using advanced interferometry, revealing its distorted surface due to rapid rotation. Standard models failed to explain the observed gravity darkening, suggesting complex rotation patterns.

Area of Science:

  • * Astrophysics
  • * Stellar Physics
  • * Optical Interferometry

Background:

  • * Understanding stellar surfaces is crucial for stellar physics.
  • * Rapidly rotating stars exhibit unique photospheric properties.
  • * Optical long-baseline interferometry offers high-resolution stellar surface imaging.

Purpose of the Study:

  • * To construct a high-resolution near-infrared image of the rapidly rotating star Altair.
  • * To investigate the effects of rapid rotation on stellar photospheres.
  • * To test standard stellar models against observational data.

Main Methods:

  • * Employed optical long-baseline interferometry.
  • * Achieved sub-milliarcsecond resolution imaging.
  • * Focused on near-infrared wavelengths.

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Main Results:

  • * Generated a near-infrared image of Altair with unprecedented resolution.
  • * Clearly observed significant gravity darkening across the stellar photosphere.
  • * Detected a high degree of photospheric distortion.

Conclusions:

  • * Standard models of uniformly rotating stars are insufficient to explain Altair's observed surface.
  • * The findings suggest the presence of differential rotation or non-standard gravity-darkening laws.
  • * Further research is needed to refine stellar rotation and gravity-darkening models.