Multiply-deuterated species in prestellar cores

Abstract

We have studied the ortho, para, and, in the case of D + , meta forms of the multiply-deuterated isotopes of H + , under physical conditions believed to be appropriate to pre-protostellar cores. As deuterons have integral nuclear spin, I = 1, Bose-Einstein statistical laws apply. Having extended the network of chemical reactions used in our previous study (Walmsley et al. 2004), we have calculated the population densities of ortho- and para-D2H + and of ortho- and meta-D + . In the former case, comparison is made with the recent observations of para-D2H + in the prestellar core 16293E (Vastel et al. 2004). Using radiative transition probabilities computed by Ramanlal & Tennyson (2004), we have predicted the intensities of the near infrared vibrational transitions of the deuterated isotopes of H + . Many of these transitions can be observed, in absorption, only from above the Earth's atmosphere, but some might be detectable through atmospheric windows.