A new ultrahigh vacuum experiment is described to study atom and radical addition reactions in interstellar ice analogues for astronomically relevant temperatures. The new setup – SURFace REaction SImulation DEvice (SURFRESIDE2) – allows a systematic investigation of solid state pathways resulting in the formation of molecules of astrophysical interest. The implementation of a double beam line makes it possible to expose deposited ice molecules to different atoms and/or radicals sequentially or at the same time. Special efforts are made to perform experiments under fully controlled laboratory conditions, including precise atom flux determinations, in order to characterize reaction channels quantitatively. In this way, we can compare and com...
Thin film growth and desorption behaviour of simple molecules have been studied by means of surface...
Carbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface coole...
Our laboratory research program is about the formation of molecules on dust grains analogues in cond...
A new ultrahigh vacuum experiment is described to study atom and radical addition reactions in inter...
Solid CO2 has been observed towards both active star forming regions and quiescent clouds (Gerakines...
It has been a long standing problem in astrochemistry to explain how molecules can form in a highly ...
Although several research groups have studied the formation of H2 on interstellar dust grains using ...
Although several research groups have studied the formation of H2 on interstellar dust grains using ...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
The region of space between stars, the interstellar medium, has been found to contain over 160 chemi...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Thin film growth and desorption behaviour of simple molecules have been studied by means of surface...
Carbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface coole...
Our laboratory research program is about the formation of molecules on dust grains analogues in cond...
A new ultrahigh vacuum experiment is described to study atom and radical addition reactions in inter...
Solid CO2 has been observed towards both active star forming regions and quiescent clouds (Gerakines...
It has been a long standing problem in astrochemistry to explain how molecules can form in a highly ...
Although several research groups have studied the formation of H2 on interstellar dust grains using ...
Although several research groups have studied the formation of H2 on interstellar dust grains using ...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
The region of space between stars, the interstellar medium, has been found to contain over 160 chemi...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
To explain the existence and observations of prebiotic molecules in interstellar and protostellar en...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Thin film growth and desorption behaviour of simple molecules have been studied by means of surface...
Carbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface coole...
Our laboratory research program is about the formation of molecules on dust grains analogues in cond...