Chemical abundances in the protoplanetary disc LV 2 (Orion): clues to the causes of the abundance anomaly in H iiregions

Author: Tsamis Y. G.   Walsh J. R.   Vílchez J. M.   Péquignot D.  

Publisher: Oxford University Press

ISSN: 0035-8711

Source: Monthly Notices of the Royal Astronomical Society, Vol.412, Iss.2, 2011-04, pp. : 1367-1380

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content