Cite
HARVARD Citation
Ercolano, B. et al. (2014). The Ṁ–M* relation of pre-main-sequence stars: a consequence of X-ray driven disc evolution. Monthly notices of the Royal Astronomical Society. 439 (1), pp. 256-263. [Online].
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Ercolano, B. et al. (2014). The Ṁ–M* relation of pre-main-sequence stars: a consequence of X-ray driven disc evolution. Monthly notices of the Royal Astronomical Society. 439 (1), pp. 256-263. [Online].