Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S287(8), p. 176-177, 2012
DOI: 10.1017/s1743921312006874
Full text: Unavailable
AbstractIn order to answer this question, we examine the relationship between the two sites of maser activity in G357.96-0.16. We also propose future observations for examining the dust properties of this interesting region of massive star formation.