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The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Its membership of about 7,000 individuals also includes physicists, mathematicians, geologists, engineers, and others whose research and educational interests lie within the broad spectrum of subjects comprising contemporary astronomy. The mission of the AAS is to enhance and share humanity's scientific understanding of the universe.

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Molecular Carbon Chains and Rings in TMC-1

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© 2001. The AmericanAstronomical Society. All rights reserved. Printed inU.S.A.
,,Citation David Fosséet al 2001ApJ552 168DOI 10.1086/320471

David Fossé

AFFILIATIONS

Depto Física Molecular, Instituto de Estructura de la Materia, Consejo Superior de Investigaciones Científicas, Serrano 121, E-28006 Madrid, Spain

Laboratoire de Radioastronomie Millimétrique, Observatoire de Paris and Ecole Normale Supérieure, 24 rue Lhomond, F-75231 Paris, CEDEX 05, France

José Cernicharo

AFFILIATIONS

Depto Física Molecular, Instituto de Estructura de la Materia, Consejo Superior de Investigaciones Científicas, Serrano 121, E-28006 Madrid, Spain

Maryvonne Gerin

AFFILIATIONS

Laboratoire de Radioastronomie Millimétrique, Observatoire de Paris and Ecole Normale Supérieure, 24 rue Lhomond, F-75231 Paris, CEDEX 05, France

Pierre Cox

AFFILIATIONS

Institut d’Astrophysique Spatiale, Université de Paris-Sud, Bâtiment 121, F-91405 Orsay, France

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Dates

  1. Received2000 April 18
  2. Accepted2001 January 3
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0004-637X/552/1/168

Abstract

We present mapping results in several rotational transitions of HC3N, C6H, both cyclic and linear C3H2 and C3H, toward the cyanopolyyne peak of the filamentary dense cloud TMC-1 using the IRAM 30 m and MPIfR 100 m telescopes. The spatial distribution of the cumulene carbon chain propadienylidene H2CCC (hereafterl-C3H2) is found to deviate significantly from the distributions of the cyclic isomerc-C3H2, HC3N, and C6H, which, in turn, look very similar. The cyclic over linear abundance ratio of C3H2 increases by a factor of 3 across the filament, with a value of 28 at the cyanopolyyne peak. This abundance ratio is an order of magnitude larger than the range (3-5) we observed in the diffuse interstellar medium. The cyclic over linear abundance ratio of C3H also varies by ~2.5 in TMC-1, reaching a maximum value (13) close to the cyanopolyyne peak. These behaviors might be related to competitive processes between ion-neutral and neutral-neutral reactions for cyclic and linear species.

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10.1086/320471

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