REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods

@article{Frasca2009REMNA,
  title={REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods},
  author={A. Frasca and E. Covino and Loredana Spezzi and J. M. Alcal{\`a} and Ettore Marilli and Gaabor Furesz and Davide Gandolfi},
  journal={Astronomy and Astrophysics},
  year={2009}
}
Aims. We aim at determining the rotational periods and the starspot properties in very young low-mass stars belonging to the Ori OB1c star forming region, contributing to the study of the angular momentum and magnetic activity evolution in these objects. Methods. We performed an intensive photometric monitoring of the PMS stars falling in a field of about 10 0 � 10 0 in the vicinity of the Orion Nebula Cluster (ONC), also containing the BD eclipsing system 2MASSJ05352184-0546085. Photometric… 
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