The photodissociation dynamics of astrophysically relevant
propyl
derivatives (C3H7X; X = CN, OH, HCO) at 157
nm exploiting an ultracompact velocity map imaging (UVMIS) setup has
been reported. The successful operation of UVMIS allowed the exploration
of the 157 nm photodissociation of six (iso)propyl systemsn/i-propyl cyanide (C3H7CN), n/i-propyl alcohol (C3H7OH), and (iso)butanal
(C3H7CHO)to explore the C3H7 loss channel. The distinct center-of-mass translational
energy distributions for the i-C3H7X (X= CN, OH, HCO) could be explained through preferential
excitation of the low frequency C–H bending modes of the formyl
moiety compared to the higher frequency stretching of the cyano and
hydroxy moieties. Although the ionization energy of the n-C3H7 radical exceeds the energy of a 157 nm
photon, C3H7
+ was observed in the n-C3H7X (X = CN, OH, HCO) systems
as a result of photoionization of vibrationally “hot” n-C3H7 fragments, photoionization
of i-C3H7 after a hydrogen
shift in vibrationally “hot” n-C3H7 radicals, and/or two-photon ionization. Our
experiments reveal that at least the isopropyl radical (i-C3H7) and possibly the normal propyl radical
(n-C3H7) should be present
in the interstellar medium and hence searched for by radio telescopes.