Volume 426, Number 1, October IV 2004
|Page(s)||219 - 227|
|Section||Stellar structure and evolution|
|Published online||05 October 2004|
The abundance of S in IRC+10216 and its production in the Galaxy*
Instituto de Radioastronomía Milimétrica, Avda. Divina Pastora 7, Local 20, 18012 Granada, Spain e-mail: firstname.lastname@example.org
2 Max-Planck-Institut für Chemie, Becherweg 27, 55128 Mainz, Germany
3 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
4 Instituto de la Estructura de la Materia, Dept. de Astronomía Molecular e Infrarroja, Serrano 113, 28006 Madrid, Spain
5 Dipartimento di Fisica Generale dell'Università di Torino, Via Pietro Giuria 1, 10125 Torino, Italy
6 Centre for Stellar and Planetary Sciences, Monash University, Melbourne 3800, Australia
Accepted: 21 June 2004
The and rotational lines of the rare isotopomer C36S and the and transitions of Si36S were detected in the carbon star IRC+10216 (CW Leo). These are the first detections of 36S-bearing molecules in a star and the first spectroscopic detection of Si36S. From a comparison of 34S- and 36S-bearing isotopomers, the 34S/36S isotopic ratio is 107(). This value is comparable to values in the interstellar medium of the inner Galactic disk (115) but is smaller than the solar value of 288 (Ding et al. [CITE]). The increase of the 36S abundance relative to 34S only qualitatively follows model predictions of a low mass AGB star. Quantitative agreement of the observed 34S/36S ratio with the stellar models can be reached if the age of IRC+10216 and Galactic chemical evolution are taken into account. Other less likely possibilities are the presence of considerable inhomogeneities in the interstellar medium and either IRC+10216 or the Sun started with a peculiar 36S abundance. Other production mechanisms potentially capable of enhancing the Galactic interstellar medium are discussed. From the observed line density toward IRC+10216 and toward Galactic star forming regions, we estimate the confusion limit toward those sources.
Key words: nuclear reactions, nucleosynthesis, abundances / stars: abundances / stars: AGB and post-AGB / stars: individual: IRC+10216 / ISM: abundances / radio lines: stars
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.