The Accretion Process in the DQ Tau Binary System

@article{Fiorellino2022TheAP,
  title={The Accretion Process in the DQ Tau Binary System},
  author={Eleonora Fiorellino and S. Park and {\'A}. K{\'o}sp{\'a}l and P{\'e}ter {\'A}brah{\'a}m},
  journal={The Astrophysical Journal},
  year={2022},
  volume={928}
}
Mass accretion from the circumstellar disk onto the protostar is a fundamental process during star formation. Measuring the mass accretion rate is particularly challenging for stars belonging to binary systems, because it is often difficult to discriminate which component is accreting. DQ Tau is an almost equal-mass spectroscopic binary system where the components orbit each other every 15.8 days. The system is known to display pulsed accretion, i.e., the periodic modulation of the accretion by… 

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