0000000000391280

AUTHOR

Maryvonne Gerin

showing 2 related works from this author

Detection of deuterated molecules, but not of lithium hydride, in the z = 0.89 absorber toward PKS 1830−211

2020

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lithium hydride, 7LiH, at redshift z=0.89 in the spiral galaxy intercepting the line of sight to the quasar PKS1830-211. We used ALMA to observe several submillimeter lines of ND, NH2D, and HDO, and their related isotopomers NH2, NH3, and H2^18O, in absorption against the southwest image of the quasar, allowing us to derive XD/XH abundance ratios. The absorption spectra mainly consist of two distinct narrow velocity components for which we find remarkable differences. One velocity component shows XD/XH abundances that…

Absorption spectroscopyquasarsFOS: Physical scienceschemistry.chemical_elementAstrophysics01 natural scienceschemistry.chemical_compound0103 physical sciencesISM -galaxiesgalaxiesindividual010303 astronomy & astrophysicsLine (formation)Physics[PHYS]Physics [physics]Spiral galaxy010308 nuclear & particles physicsmolecules -radio linesAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshift3. Good healthPKS 1830−211 -galaxiesabundances -ISMDeuteriumchemistry13. Climate actionSpace and Planetary ScienceLithium hydride[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Lithium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorption lines -quasars
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The hyperfine structure in the rotational spectrum of CF+

2012

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter lines. The origin of this double-peak profile may be kinematic or spectroscopic. Aims. We investigate the effect of hyperfine interactions due to the fluorine nucleus in CF+ on the rotational transitions. Methods. We compute the fluorine spin rotation constant of CF+ using high-level quantum chemical methods and determine the relative positions and intensities of each hyperfine component. This information is used to fit the theoretical hyperfine components to the observed CF+ line profiles, thereby employing the h…

AstrochemistryFOS: Physical sciencesContext (language use)Astrophysics010402 general chemistryRotation01 natural sciencesISM: clouds0103 physical sciencesSpin (physics)010303 astronomy & astrophysicsHyperfine structureAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsNebularadio lines: ISMastrochemistryAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesISM: molecules0104 chemical sciences[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ISM: individual objects: Horsehead nebula[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Atomic physicsBar (unit)
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