Zobrazeno 1 - 10
of 143
pro vyhledávání: '"Gianfranco Vidali"'
Autor:
Jiao He, Paula Caroline Pérez Rickert, Tushar Suhasaria, Orianne Sohier, Tia Bäcker, Dimitra Demertzi, Gianfranco Vidali, Thomas K. Henning
The diffusion of molecules on interstellar grain surfaces is one of the most important driving forces for the molecular complexity in the interstellar medium. Due to the lack of laboratory measurements, astrochemical modeling of grain surface process
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::089a01a6bdaac1414ccfc8ef346bdb8d
http://arxiv.org/abs/2302.08628
http://arxiv.org/abs/2302.08628
Publikováno v:
The journal of physical chemistry. A. 126(12)
Mid-infrared studies of fundamental modes of ices of pure CH
Autor:
Jiao He, Giulia Perotti, Shahnewaz M. Emtiaz, Francis E. Toriello, Adwin Boogert, Thomas Henning, Gianfranco Vidali
Publikováno v:
Astronomy & Astrophysics. 668:A76
CO is one of the most abundant ice components on interstellar dust grains. When it is mixed with amorphous solid water (ASW) or located on its surface, an absorption band of CO at 2152 cm$^{-1}$ is always present in laboratory measurements. This spec
Publikováno v:
ACS Earth and Space Chemistry. 4:488-490
Publikováno v:
The Journal of Physical Chemistry A. 124:552-559
Infrared spectroscopy was employed to study thin films of solid methane at low temperatures. We report new measurements of temporal changes of infrared spectra of methane ice in the ν3 and ν4 bands...
Publikováno v:
Physical Chemistry Chemical Physics. 20:19750-19758
We studied the isotopic composition of ozone formed at low (3-10 K) temperature via O + O2 solid state reactions using a partially dissociated 16O/16O2 : 18O/18O2 = 1 : 1 mixture. The ozone ice has an isotopic abundance that differs from the statisti
Autor:
Jiao He, Gianfranco Vidali
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 473:860-866
Carbon dioxide is abundant in ice mantles of dust grains; some is found in the pure crystalline form as inferred from the double peak splitting of the bending profile at about 650 cm$^{-1}$. To study how CO$_2$ segregates into the pure form from wate
Autor:
Jiao He, Shahnewaj M. Emtiaz, A. R. Clements, Gianfranco Vidali, Francis Toriello, Robin T. Garrod
The need to characterize ices coating dust grains in dense interstellar clouds arises from the importance of ice morphology in facilitating the diffusion and storage of radicals and reaction products in ices, a well-known place for the formation of c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::723d5e042fa8d887f56c51904a0b8da9
Publikováno v:
Astrophysical Journal, 869(1), 41
Analyses of infrared signatures of CO$_2$ in water dominated ices in the ISM can give information on the physical state of CO$_2$ in icy grains and on the thermal history of the ices themselves. In many sources, CO$_2$ was found in the `pure' crystal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a67a39af6edb5eca2636bae7a026732
http://arxiv.org/abs/1810.07754
http://arxiv.org/abs/1810.07754
The diffusion of atoms and molecules in ices covering dust grains in dense clouds in interstellar space is an important but poorly characterized step in the formation of complex molecules in space. Here we report the measurement of diffusion of simpl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be105e0ea7f219354b3fd4d3d2574cad
http://arxiv.org/abs/1806.06980
http://arxiv.org/abs/1806.06980