| Full text | |
| Author(s): |
Total Authors: 2
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| Affiliation: | [1] Univ Vale Paraiba, Inst Pesquisa & Desenvolvimento, BR-12244000 Sao Jose Dos Campos, SP - Brazil
Total Affiliations: 1
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| Document type: | Journal article |
| Source: | ASTROPHYSICAL JOURNAL; v. 803, n. 1 APR 10 2015. |
| Web of Science Citations: | 6 |
| Abstract | |
We present a study of the effects of high energy cosmic rays (CRs) over the astrophysical ices, observed toward the embedded class I protostar Elias 29, by using computational modeling and laboratory data. Its spectrum was observed with the Infrared Space Observatory (ISO) covering 2.3-190 mu m. The modeling employed the three-dimensional Monte Carlo radiative transfer code RADMC-3D and laboratory data of bombarded ice grains by CR analogs and unprocessed ices (not bombarded). We are assuming that Elias 29 has a self-irradiated disk with inclination i = 60:0, surrounded by an envelope with a bipolar cavity. The results show that absorption features toward Elias 29 are better reproduced by assuming a combination between unprocessed astrophysical ices at low temperature (H2O, CO, CO2) and bombarded ices (H2O: CO2) by high energy CRs. Evidences of the ice processing around Elias 29 can be observed by the good fitting around 5.5-8.0 mu m, by polar and apolar ice segregation in 15.15-15.25 mu m, and by the presence of the CH4 and HCOOH ices. Given that non-nitrogen compounds were employed in this work, we assume that absorption around 5.5-8.0 mu m should not be associated with the NH4+ ion (see the 2003 work of Shutte \& Khanna), but more probably with aliphatic ethers (e.g., R1-OCH2-R2), CH3CHO, and related species. The results obtained in this paper are important because they show that the environment around protostars is better modeled considering processed samples and, consequently, demonstrate the chemical evolution of the astrophysical ices. (AU) | |
| FAPESP's process: | 13/07657-5 - Computational modeling of circumstellar environment of protostars by employing data of bombarded ices with cosmic rays simulated in laboratory. |
| Grantee: | Will Robson Monteiro Rocha |
| Support Opportunities: | Scholarships in Brazil - Doctorate |
| FAPESP's process: | 09/18304-0 - Synthesis and degradation of prebiotic molecular species at planetary atmospheres, comets and interstellar ice analogs |
| Grantee: | Sergio Pilling Guapyassu de Oliveira |
| Support Opportunities: | Research Grants - Young Investigators Grants |