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تسجيل مستخدم جديدAnomalous eclipses of the young star RW Aur A
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Results of UBVRIJHKLM photometry, VRI polarimetry and optical spectroscopy of a young star RW Aur A obtained during 2010-11 and 2014-16 dimming events are presented. During the second dimming the star decreased its brightness to Delta V > 4.5 mag, polarization of its light in I-band was up to 30%, and color-magnitude diagram was similar to that of UX Ori type stars. We conclude that the reason of both dimmings is an eclipses of the star by dust screen, but the size of the screen is much larger than in the case of UXORs.
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Comparing the images of the jet of the young star RW Aur A, separated by a period of 21.3 years, we found that the outermost jets knots have emerged $approx 350$ yr ago. We argue that at that moment the jet itself has appeared and intensive accretion
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