Corpus ID: 15406216

Non coeval young multiple systems? On the pairing of protostars and T Tauri stars

@article{Duchne2003NonCY,
  title={Non coeval young multiple systems? On the pairing of protostars and T Tauri stars},
  author={Gaspard Duch{\^e}ne and Andrea GhezCaer McCabe},
  journal={arXiv: Astrophysics},
  year={2003}
}
We summarize here the observed properties of ``infrared companions'' to T Tauri stars and argue that their observational properties are identical to those of Class I sources. They may therefore be embedded protostars in a much earlier evolutionary phase than T Tauri stars, in which case these multiple systems are significantly non-coeval as opposed to the majority of young binary systems. They would have formed through a different mechanism than core fragmentation. The only distinction between… Expand
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