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pro vyhledávání: '"Shalabeia, Osama"'
The chemical complexity in low-metallicity hot cores has been confirmed by observations. We investigate the effect of varying physical parameters, such as temperature, density and the cosmic ray ionisation rate (CRIR), on the molecular abundance evol
Externí odkaz:
http://arxiv.org/abs/2407.06791
Autor:
Awad, Zainab, Shalabeia, Osama M.
Publikováno v:
Astrophys Space Sci (2017) 362:83
We present the first gas-grain astrochemical model of the NGC 2264 CMM3 protostellar core. The chemical evolution of the core is affected by changing its physical parameters such as the total density and the amount of gas-depletion onto grain surface
Externí odkaz:
http://arxiv.org/abs/1703.04632