Polarización óptica de NGC 6231, evidencia de fenómenos energéticos
In a typical young open cluster the polarimetric data shows, for normal stars, that the distribution of angles of the polarization vectors can be describe by a fixed value that caracterizes the cluster. Individual stars show some scatter over this mean angle because of fluctuations in the interstellar medium (ISM), variations in the magnetic field
Feinstein, C. et al.
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2002