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Interstellar medium. Pseudo-three-dimensional maps of the diffuse interstellar band at 862 nm.

Identifieur interne : 003565 ( PubMed/Corpus ); précédent : 003564; suivant : 003566

Interstellar medium. Pseudo-three-dimensional maps of the diffuse interstellar band at 862 nm.

Auteurs : Janez Kos ; Tomaž Zwitter ; Rosemary Wyse ; Olivier Bienaymé ; James Binney ; Joss Bland-Hawthorn ; Kenneth Freeman ; Brad K. Gibson ; Gerry Gilmore ; Eva K. Grebel ; Amina Helmi ; Georges Kordopatis ; Ulisse Munari ; Julio Navarro ; Quentin Parker ; Warren A. Reid ; George Seabroke ; Sanjib Sharma ; Arnaud Siebert ; Alessandro Siviero ; Matthias Steinmetz ; Fred G. Watson ; Mary E K. Williams

Source :

RBID : pubmed:25124434

Abstract

The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spectra of stars. Understanding their origin in the interstellar medium is one of the oldest problems in astronomical spectroscopy, as DIBs have been known since 1922. In a completely new approach to understanding DIBs, we combined information from nearly 500,000 stellar spectra obtained by the massive spectroscopic survey RAVE (Radial Velocity Experiment) to produce the first pseudo-three-dimensional map of the strength of the DIB at 8620 angstroms covering the nearest 3 kiloparsecs from the Sun, and show that it follows our independently constructed spatial distribution of extinction by interstellar dust along the Galactic plane. Despite having a similar distribution in the Galactic plane, the DIB 8620 carrier has a significantly larger vertical scale height than the dust. Even if one DIB may not represent the general DIB population, our observations outline the future direction of DIB research.

DOI: 10.1126/science.1253171
PubMed: 25124434

Links to Exploration step

pubmed:25124434

Le document en format XML

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<name sortKey="Navarro, Julio" sort="Navarro, Julio" uniqKey="Navarro J" first="Julio" last="Navarro">Julio Navarro</name>
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<nlm:affiliation>University of Victoria, Victoria BC, Canada V8P 5C2.</nlm:affiliation>
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<name sortKey="Parker, Quentin" sort="Parker, Quentin" uniqKey="Parker Q" first="Quentin" last="Parker">Quentin Parker</name>
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<div type="abstract" xml:lang="en">The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spectra of stars. Understanding their origin in the interstellar medium is one of the oldest problems in astronomical spectroscopy, as DIBs have been known since 1922. In a completely new approach to understanding DIBs, we combined information from nearly 500,000 stellar spectra obtained by the massive spectroscopic survey RAVE (Radial Velocity Experiment) to produce the first pseudo-three-dimensional map of the strength of the DIB at 8620 angstroms covering the nearest 3 kiloparsecs from the Sun, and show that it follows our independently constructed spatial distribution of extinction by interstellar dust along the Galactic plane. Despite having a similar distribution in the Galactic plane, the DIB 8620 carrier has a significantly larger vertical scale height than the dust. Even if one DIB may not represent the general DIB population, our observations outline the future direction of DIB research.</div>
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<AbstractText>The diffuse interstellar bands (DIBs) are absorption lines observed in visual and near-infrared spectra of stars. Understanding their origin in the interstellar medium is one of the oldest problems in astronomical spectroscopy, as DIBs have been known since 1922. In a completely new approach to understanding DIBs, we combined information from nearly 500,000 stellar spectra obtained by the massive spectroscopic survey RAVE (Radial Velocity Experiment) to produce the first pseudo-three-dimensional map of the strength of the DIB at 8620 angstroms covering the nearest 3 kiloparsecs from the Sun, and show that it follows our independently constructed spatial distribution of extinction by interstellar dust along the Galactic plane. Despite having a similar distribution in the Galactic plane, the DIB 8620 carrier has a significantly larger vertical scale height than the dust. Even if one DIB may not represent the general DIB population, our observations outline the future direction of DIB research.</AbstractText>
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