Phosphorus is a crucial element in biochemistry, especially the P-O bond, which is key for the formation of the backbone of the deoxyribonucleic acid. So far, PO has only been detected towards the envelope of evolved stars, and never towards star-forming regions. We report the first detections of PO towards two massive star-forming regions, W51 e1/e2 and W3(OH), using data from the IRAM 30m telescope. PN has also been detected towards the two regions. The abundance ratio PO/PN is 1.8 and 3 for W51 and W3(OH), respectively. Our chemical model indicates that the two molecules are chemically related and are formed via gas-phase ion-molecule and neutral-neutral reactions during the cold collapse. The molecules freeze out onto grains at the end of the collapse and desorb during the warm-up phase once the temperature reaches 35 K. Similar abundances of the two species are expected during a period of 5x10^{4} yr at the early stages of the warm-up phase, when the temperature is in the range 35-90 K. The observed molecular abundances of 10^{-10} are predicted by the model if a relatively high initial abundance of 5x10^{-9} of depleted phosphorus is assumed.
@article{arxiv.1605.06109,
title = {First detections of the key prebiotic molecule PO in star-forming regions},
author = {V. M. Rivilla and F. Fontani and M. T. Beltrán and A. Vasyunin and P. Caselli and J. Martín-Pintado and R. Cesaroni},
journal= {arXiv preprint arXiv:1605.06109},
year = {2016}
}
Comments
9 pages, 7 figures, 6 tables. Accepted in The Astrophysical Journal