Are interstellar ices porous, and how do the pores collapse?
2015 ◽
Vol 11
(A29A)
◽
Keyword(s):
Amorphous solid water (ASW) is of great importance in astrochemistry as it has been detected in star forming regions, comets, and cold solar-system objects. A key property of ASW is its porous nature (with the extent of porosity reflecting the formation and growth conditions) and the subsequent pore collapse when the ice is heated. If interstellar ices are porous there are huge implications to both the process of planet formation and the budgets of molecular gas in the solid and gas phases. It is therefore vital to understand ASW porosity over astronomically relevant conditions in order to effectively model its potential effects on these processes.
2015 ◽
Vol 11
(A29A)
◽
pp. 271-274
Nitrogen and hydrogen fractionation in high-mass star-forming cores from observations of HCN and HNC
2018 ◽
Vol 609
◽
pp. A129
◽
Keyword(s):
2016 ◽
Vol 11
(S321)
◽
pp. 214-216
Keyword(s):
1987 ◽
Vol 115
◽
pp. 181-181
◽
Keyword(s):
1999 ◽
Vol 190
◽
pp. 67-73
◽
Keyword(s):
1997 ◽
Vol 159
◽
pp. 439-440
◽
2019 ◽
Vol 15
(S350)
◽
pp. 368-369
2008 ◽
Vol 4
(S256)
◽
pp. 215-226
Keyword(s):