期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 688, 期 2, 页码 L83-L86出版社
IOP PUBLISHING LTD
DOI: 10.1086/595583
关键词
circumstellar matter; ISM: molecules; radio lines: ISM; stars: AGB and post-AGB; stars: individual (IRC+10216)
We report the detection in the envelope of the C-rich star IRC + 10216 of four series of lines with harmonically related frequencies: B1389, B1390, B1394, and B1401. The four series must arise from linear molecules with mass and size close to those of C6H and C5N. Three of the series have half-integer rotational quantum numbers; we assign them to the (2)Delta and (2)Sigma(-) vibronic states of C6H in its lowest (nu(11)) bending mode. The fourth series, B1389, has integer J with no evidence of fine or hyperfine structure; it has a rotational constant of 1388.860(2) MHz and a centrifugal distortion constant of 33(1) Hz; it is almost certainly the C5N- anion.
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