Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations
Identifieur interne : 000205 ( France/Analysis ); précédent : 000204; suivant : 000206Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations
Auteurs : Mario Hernandez-Vera [France]Source :
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Abstract
Accurate molecular data, such collisional rate coefficients, are essential to model molecular lines and then to estimate molecular abundances in the interstellar medium (ISM). For this reason, we have used quantum approximations to study the rotational (de-)excitation of AlCN(1Σ), AlNC(1Σ), MgCN(2Σ), MgNC(2Σ), SiCN(2∏) and SiNC(2∏) molecules by collisions with He, as a model of H2. We have also considered the rotational (de-)excitation of HCN(1Σ) molecules by ortho-H2 and para-H2 molecules.Then, we have performed radiative transfer calculations in order to estimate the relative abundances of cyanide/isocyanide species in the ISM. The impact of our molecular data in the simulation of molecular emissions is discussed. Despite the similar spectroscopic characteristics of the isomers, this work demonstrates the importance of conducting separate collisional rate calculations for each isomer in order to obtain their abundances.
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<front><div type="abstract" xml:lang="en">Accurate molecular data, such collisional rate coefficients, are essential to model molecular lines and then to estimate molecular abundances in the interstellar medium (ISM). For this reason, we have used quantum approximations to study the rotational (de-)excitation of AlCN(1Σ), AlNC(1Σ), MgCN(2Σ), MgNC(2Σ), SiCN(2∏) and SiNC(2∏) molecules by collisions with He, as a model of H2. We have also considered the rotational (de-)excitation of HCN(1Σ) molecules by ortho-H2 and para-H2 molecules.Then, we have performed radiative transfer calculations in order to estimate the relative abundances of cyanide/isocyanide species in the ISM. The impact of our molecular data in the simulation of molecular emissions is discussed. Despite the similar spectroscopic characteristics of the isomers, this work demonstrates the importance of conducting separate collisional rate calculations for each isomer in order to obtain their abundances.</div>
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