Abstract
We analyse evolutionary tracks at young ages for low mass stars with masses m ≤ 1.4 M ⊙ and brown dwarfs down to one mass of Jupiter. We analyse current theoretical uncertainties due to initial conditions. Simple tests on initial conditions show the high uncertainties of models at ages ≲ 1 Myr.
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CITATION STYLE
APA
Baraffe, I., Chabrier, G., Allard, F., & Hauschildt, P. (2003). Evolutionary Models for Low Mass Stars and Brown Dwarfs at Young Ages. Symposium - International Astronomical Union, 211, 41–50. https://doi.org/10.1017/s0074180900210243
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