About the modelling of the SED for the inner boundary of protoplanetary discs at the lower stellar mass regime
ABSTRACT In order to improve the physical interpretation about innermost dusty regions in protoplanetary discs around brown dwarf (BD), and even very low mass star (VLMS), we present a grid of models taking into account two different sets: (i) The set called standard model, that simulates an axisymm...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2021-10, Vol.506 (4), p.5361-5372 |
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| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
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