English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/185224
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:


Discovery of SiCSi in IRC+10216: A missing link between gas and dust carriers of Si-C bonds

AuthorsCernicharo, José ; McCarthy, M. C.; Gottlieb, C. A.; Agúndez, Marcelino ; Velilla Prieto, L. ; Baraban, J. H.; Changala, P. B.; Guélin, M.; Kahane, C.; Martin-Drumel, M. A.; Patel, N. A.; Reilly, N. J.; Stanton, J. F.; Quintana-Lacaci, G. ; Thorwirth, S.; Young, K. H.
KeywordsStars: carbon
Stars: AGB and post-AGB
Stars: individual (IRC, 10216)
Issue Date2-Jun-2015
PublisherAmerican Astronomical Society
CitationThe Astrophysical Journal 806 (2015)
AbstractWe report the discovery in space of a disilicon species, SiCSi, from observations between 80 and 350 GHz with the IRAM 30 m radio telescope. Owing to the close coordination between laboratory experiments and astrophysics, 112 lines have now been detected in the carbon-rich star CW Leo. The derived frequencies yield improved rotational and centrifugal distortion constants up to sixth order. From the line profiles and interferometric maps with the Submillimeter Array, the bulk of the SiCSi emission arises from a region of 6'' in radius. The derived abundance is comparable to that of SiC2. As expected from chemical equilibrium calculations, SiCSi and SiC2 are the most abundant species harboring a Si−C bond in the dust formation zone and certainly both play a key role in the formation of SiC dust grains.
Publisher version (URL)https://doi.org/10.1088/2041-8205/806/1/L3
Identifiersdoi: 10.1088/2041-8205/806/1/L3
e-issn: 2041-8213
issn: 2041-8205
Appears in Collections:(ICMM) Artículos
Files in This Item:
File Description SizeFormat 
accesoRestringido.pdf15,38 kBAdobe PDFThumbnail
Show full item record
Review this work

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.