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Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations

Identifieur interne : 000205 ( France/Analysis ); précédent : 000204; suivant : 000206

Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations

Auteurs : Mario Hernandez-Vera [France]

Source :

RBID : Hal:tel-01131371

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English descriptors

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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Hal:tel-01131371

Le document en format XML

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<title xml:lang="en">Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations</title>
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<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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   |wiki=    Wicri/France
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   |texte=   Towards the understanding of cyanide/isocyanide abundances : inelastic collisions and radiative transfer calculations
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