Electron Abundance in Protostellar Cores

Details Electron Abundance in Protostellar Cores Electron Abundance in Protostellar Cores

2004-06-23

arxiv.org/abs/astro-ph/0406500v1

Astrophys.J. 614 (2004) 203-210

Astronomy and Astrophysics

Astrophysics

25 pages, 9 figures. Astrophysical Journal, in press

Scientific paper

10.1086/423659

The determination of the fractional electron abundance, Xe, in protostellar cores relies on observations of molecules, such as DCO+, H13CO+ and CO, and on chemical models to interpret their abundance. Studies of protostellar cores have revealed significant variations of Xe from core to core within a range 10^-8

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