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The dynamics of red supergiant winds
2002
Symposium - International astronomical union
During the red supergiant (RSG) stage of massive star evolution, emission from dust and molecules allows the copious stellar winds to be studied in great detail. This help us understand not only the evolutionary stages of the star (which are highly dependent on mass loss rates), but also the morphology of the eventual supernova remnant. Maser emission from OH and H2O has been mapped with milli-arcsec resolution (using MERLIN and the EVN/global VLBI) around RSG including VY CMa, S Per and VX
doi:10.1017/s0074180900222596
fatcat:nowsi7xem5gg7apxoezzkvhccm