The model of a young star with a low-mass secondary component (q = M2/M1
Original languageEnglish
Pages (from-to)521-524
JournalProceedings of the International Astronomical Union
Volume7
Issue number282
DOIs
StatePublished - 2012

    Research areas

  • accretion, accretion discs, hydrodynamics, numerical method, close binaries

ID: 5400154