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Modeling long carbon-chain species formation with porous multiphase models
Song, Ziwen1; Chang, Qiang1; Meng, Qingkuan1; Zhang, Xia2
2024-10-25
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume691Pages:A40
Contribution Rank2
AbstractContext. Recent studies show that multiphase models trap too many volatile species such as CH4 inside ice mantles, so they usually underestimate the abundances of long carbon-chain species observed toward warm carbon-chain chemistry (WCCC) sources. Aims. We propose a new multiphase model that allows more volatile species to diffuse out of the ice mantle upon warming. The new multiphase model is used to study the synthesis of long carbon-chain molecules in WCCC sources. Methods. We included porous structure in the ice mantles. The porous structure can enlarge the active layers of ice mantles so that fewer volatile species are trapped. The porous multiphase models were simulated using an accelerated Gillespie algorithm. Results. The abundances of long carbon-chain species predicted by the porous multiphase models can be more than one order of magnitude higher than those predicted by the multiphase model at temperatures relevant to WCCC sources. Moreover, the porous multiphase models predict more abundant long carbon-chain species as the porosity of the ice mantles increases. On the other hand, the two-phase model still estimates higher long carbon-chain species abundances than the porous multiphase models do. The abundances of long carbon-chain species predicted by our porous multiphase models agree reasonably well with observations toward three WCCC sources, L483, L1527, and B228. Conclusions. Our porous multiphase model solves the problem of too many volatile species being trapped in ice mantles in the multiphase models.
Keywordastrochemistry ISM: abundances ISM: molecules
DOI10.1051/0004-6361/202450647
Indexed BySCI
Language英语
WOS KeywordGAS-GRAIN CHEMISTRY ; MONTE-CARLO TREATMENT ; INTERSTELLAR ICE ; PROTOSTELLAR CORES ; BULK DIFFUSION ; SIMULATIONS ; PRESTELLAR ; MOLECULES ; CLOUDS ; PHASE
Funding ProjectNational Natural Science Foundation of China[12173023] ; National Natural Science Foundation of China[12203091]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001342109500025
PublisherEDP SCIENCES S A
Funding OrganizationNational Natural Science Foundation of China
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7146
Collection射电天文研究室_天体化学研究团组
Corresponding AuthorChang, Qiang
Affiliation1.Shandong Univ Technol, Sch Phys & Optoelect Engn, 266 West Xincun Rd, Zibo 255000, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
Recommended Citation
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Song, Ziwen,Chang, Qiang,Meng, Qingkuan,et al. Modeling long carbon-chain species formation with porous multiphase models[J]. ASTRONOMY & ASTROPHYSICS,2024,691:A40.
APA Song, Ziwen,Chang, Qiang,Meng, Qingkuan,&Zhang, Xia.(2024).Modeling long carbon-chain species formation with porous multiphase models.ASTRONOMY & ASTROPHYSICS,691,A40.
MLA Song, Ziwen,et al."Modeling long carbon-chain species formation with porous multiphase models".ASTRONOMY & ASTROPHYSICS 691(2024):A40.
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