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- W4289875003 startingPage "A49" @default.
- W4289875003 abstract "Context. Protostars grow from the first formation of a small seed and subsequent accretion of material. Recent theoretical work has shown that the pre-main-sequence (PMS) evolution of stars is much more complex than previously envisioned. Instead of the traditional steady, one-dimensional solution, accretion may be episodic and not necessarily symmetrical, thereby affecting the energy deposited inside the star and its interior structure." @default.
- W4289875003 created "2022-08-05" @default.
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- W4289875003 date "2017-02-24" @default.
- W4289875003 modified "2023-10-05" @default.
- W4289875003 title "Revisiting the pre-main-sequence evolution of stars" @default.
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- W4289875003 doi "https://doi.org/10.1051/0004-6361/201628260" @default.
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