Are the spin axes of stars randomly aligned within a cluster?

We investigate to what extent the spin axes of stars in young open clusters are aligned. Assuming that the spin vectors lie uniformly within a conical section, with an opening half-angle between λ= 0° (perfectly aligned) and λ= 90° (completely random), we describe a Monte Carlo modelling technique t...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2010-02, Vol.402 (2), p.1380-1390
Hauptverfasser: Jackson, R. J., Jeffries, R. D.
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Sprache:eng
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