| Tsamis et al. 2011; Chemical abundances in the protoplanetary disc LV 2 (Orion): clues to the causes of the abundance anomaly in H II regions |
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| Martes 25 de Octubre de 2011 15:29 | |||
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Tsamis, Y. G.; Walsh, J. R.; Vílchez, J. M.; Péquignot, D. Monthly Notices of the Royal Astronomical Society vol. 412, pag. 1367
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