Speaker
Description
Today thanks to the advent of large telescopes, an increasing number of gas phase complex molecules is observed in star forming regions, prestellar dense cores, circumstellar disks and winds [1, 2, 3]. Planets are formed in protoplanetary disks during the first millions of years of stellar evolution. Thus, it is important to understand if molecules observed in gas phase, are already available in the solid phase adsorbed on the surface of dust and which fraction of such molecules will end up in protoplanetary disks in newly formed planetesimal.
Among these molecules formamide (
These studies will support the interpretation of molecule observations in star forming regions with the goal of understanding the role of the grain surface in driving prebiotic chemistry in space.
[1] Beltrán, M. T. et al. 2009, The Astrophysical Journal Letters, Vol. 690
[2] Rivilla, V. M. et al. 2017, Astronomy & Astrophysics, Vol. 598
[3] Codella, C. et al. 2015, Mon. Not. R. Astron. Soc., Vol. 449
[4] Nummelin, A. et al. 1998, The Astrophysical Journal Supplement Series, Vol. 117