Grain growth and its chemical impact in the first hydrostatic core phase Article Swipe
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2403.01905
The first hydrostatic core (FHSC) phase is a brief stage in the protostellar evolution that is difficult to detect. Our goal is to characterize the chemical evolution of gas and dust during the formation of the FHSC. Moreover, we are interested in analyzing, for the first time with 3D magnetohydrodynamic (MHD) simulations, the role of grain growth in its chemistry. We postprocessed $2\times10^{5}$ tracer particles from a $\texttt{RAMSES}$ non-ideal MHD simulation using the codes $\texttt{NAUTILUS}$ and $\texttt{SHARK}$ to follow the chemistry and grain growth throughout the simulation. A great chemical inheritance is seen, as gas-phase abundances of most of the C, O, N, and S reservoirs in the hot corino at the end of the simulation match the ice-phase abundances from the prestellar phase. Additionally, interstellar complex organic molecules (iCOMs) such as methyl formate, acetaldehyde, and formamide are formed during the warm-up process. The typical grain size in the hot corino $(n_{\rm H}>10^{11}\ {\rm cm^{-3}})$ increases forty-fold during the last 30 kyr, with negligible effects on its chemical composition. At moderate densities $(10^{10}
Related Topics
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2403.01905
- https://arxiv.org/pdf/2403.01905
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4392488802
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4392488802Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.48550/arxiv.2403.01905Digital Object Identifier
- Title
-
Grain growth and its chemical impact in the first hydrostatic core phaseWork title
- Type
-
preprintOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2024Year of publication
- Publication date
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2024-03-04Full publication date if available
- Authors
-
D. Navarro-Almaida, U. Lebreuilly, P. Hennebelle, A. Fuente, B. Commerçon, Romane Le Gal, Valentine Wakelam, Maryvonne Gérin, P. Riviére-Marichalar, Leire Beitia-Antero, Y. AscasíbarList of authors in order
- Landing page
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https://arxiv.org/abs/2403.01905Publisher landing page
- PDF URL
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https://arxiv.org/pdf/2403.01905Direct link to full text PDF
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
-
https://arxiv.org/pdf/2403.01905Direct OA link when available
- Concepts
-
Core (optical fiber), Hydrostatic equilibrium, Grain growth, Phase (matter), Materials science, Hydrostatic pressure, Grain size, Chemistry, Metallurgy, Composite material, Thermodynamics, Physics, Quantum mechanics, Organic chemistryTop concepts (fields/topics) attached by OpenAlex
- Cited by
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0Total citation count in OpenAlex
- Related works (count)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.molecules | 128 |
| abstract_inverted_index.non-ideal | 68 |
| abstract_inverted_index.particles | 64 |
| abstract_inverted_index.abundances | 95, 119 |
| abstract_inverted_index.analyzing, | 42 |
| abstract_inverted_index.chemistry. | 59 |
| abstract_inverted_index.cm^{-3}})$ | 154 |
| abstract_inverted_index.forty-fold | 156 |
| abstract_inverted_index.interested | 40 |
| abstract_inverted_index.negligible | 163 |
| abstract_inverted_index.prestellar | 122 |
| abstract_inverted_index.reservoirs | 105 |
| abstract_inverted_index.simulation | 70, 115 |
| abstract_inverted_index.throughout | 84 |
| abstract_inverted_index.hydrostatic | 2 |
| abstract_inverted_index.inheritance | 90 |
| abstract_inverted_index.simulation. | 86 |
| abstract_inverted_index.characterize | 23 |
| abstract_inverted_index.composition. | 168 |
| abstract_inverted_index.interstellar | 125 |
| abstract_inverted_index.protostellar | 12 |
| abstract_inverted_index.simulations, | 51 |
| abstract_inverted_index.Additionally, | 124 |
| abstract_inverted_index.acetaldehyde, | 134 |
| abstract_inverted_index.postprocessed | 61 |
| abstract_inverted_index.H}>10^{11}\ | 152 |
| abstract_inverted_index.$2\times10^{5}$ | 62 |
| abstract_inverted_index.$\texttt{SHARK}$ | 76 |
| abstract_inverted_index.$\texttt{RAMSES}$ | 67 |
| abstract_inverted_index.$\texttt{NAUTILUS}$ | 74 |
| abstract_inverted_index.magnetohydrodynamic | 49 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 11 |
| citation_normalized_percentile |