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dc.contributor.author
Santos, Julia  
dc.contributor.author
Bronfman, Leonardo  
dc.contributor.author
Mendoza, Edgar  
dc.contributor.author
Lépine, Jacques R. D.  
dc.contributor.author
Duronea, Nicolas Urbano  
dc.contributor.author
Merello, Manuel  
dc.contributor.author
Finger, Ricardo  
dc.date.available
2023-09-08T13:03:41Z  
dc.date.issued
2022-03  
dc.identifier.citation
Santos, Julia; Bronfman, Leonardo; Mendoza, Edgar; Lépine, Jacques R. D.; Duronea, Nicolas Urbano; et al.; A Spectral Survey of CH3CCH in the Hot Molecular Core G331.512-0.103; IOP Publishing; Astrophysical Journal; 925; 1; 3-2022; 1-18  
dc.identifier.issn
0004-637X  
dc.identifier.uri
http://hdl.handle.net/11336/210900  
dc.description.abstract
A spectral survey of methyl acetylene (CH3CCH) was conducted toward the hot molecular core/outflow G331.512-0.103. Our APEX observations allowed the detection of 41 uncontaminated rotational lines of CH3CCH in the frequency range between 172 and 356 GHz. Through an analysis under the local thermodynamic equilibrium assumption, by means of rotational diagrams, we determined T exc = 50 ? 1 K, N(CH3CCH) = (7.5 ? 0.4) ? 1015 cm2, X[CH3CCH/H2] ≈ (0.8-2.8) ? 10-8, and X[CH3CCH/CH3OH] ≈ 0.42 ? 0.05 for an extended emitting region (∼10″). The relative intensities of the K = 2 and K = 3 lines within a given K-ladder are strongly negatively correlated to the transitions' upper J quantum number (r = -0.84). Pure rotational spectra of CH3CCH were simulated at different temperatures, in order to interpret this observation. The results indicate that the emission is characterized by a nonnegligible temperature gradient with upper and lower limits of ∼45 and ∼60 K, respectively. Moreover, the line widths and peak velocities show an overall strong correlation with their rest frequencies, suggesting that the warmer gas is also associated with stronger turbulence effects. The K = 0 transitions present a slightly different kinematic signature than the remaining lines, indicating that they might be tracing a different gas component. We speculate that this component is characterized by lower temperatures and therefore larger sizes. Moreover, we predict and discuss the temporal evolution of the CH3CCH abundance using a two-stage zero-dimensional model of the source constructed with the three-phase Nautilus gas-grain code.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
IOP Publishing  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Methyl acetylene  
dc.subject
Molecular outflows  
dc.subject
Hot Molecular Cores  
dc.subject
Astrochemistry  
dc.subject.classification
Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
A Spectral Survey of CH3CCH in the Hot Molecular Core G331.512-0.103  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2023-09-05T18:05:09Z  
dc.journal.volume
925  
dc.journal.number
1  
dc.journal.pagination
1-18  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: Santos, Julia. Universidade de Sao Paulo; Brasil  
dc.description.fil
Fil: Bronfman, Leonardo. Universidad de Chile. Facultad de Ciencias Físicas y Matemáticas; Chile  
dc.description.fil
Fil: Mendoza, Edgar. Universidade de Sao Paulo; Brasil. Universidade Federal do Rio de Janeiro; Brasil  
dc.description.fil
Fil: Lépine, Jacques R. D.. Universidade de Sao Paulo; Brasil  
dc.description.fil
Fil: Duronea, Nicolas Urbano. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina  
dc.description.fil
Fil: Merello, Manuel. Universidad de Chile; Chile  
dc.description.fil
Fil: Finger, Ricardo. Universidad de Chile; Chile  
dc.journal.title
Astrophysical Journal  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac36cc  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.3847/1538-4357/ac36cc