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The Astrophysical Journal
Article . 1988 . Peer-reviewed
Data sources: Crossref
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International Astronomical Union Colloquium
Article . 1988 . Peer-reviewed
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https://doi.org/10.1007/bfb003...
Part of book or chapter of book . 2006 . Peer-reviewed
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A sensitive line search in circumstellar envelopes

Authors: null Nguyen-Q-Rieu; S. Deguchi; H. Izumiura; N. Kaifu; M. Ohishi; H. Suzuki; N. Ukita;

A sensitive line search in circumstellar envelopes

Abstract

AbstractA molecular line search in the range between 85 and 89 GHz has been performed in the circumstellar envelopes of 11 evolved stars. Emissions of 29SiO J=2−1,28SiO J=2−1, HCN J=1−0, H13CN J=1−0, HC5 N J=33−32, HCO+ J=1−0 transitions and other transitions of C2 H, C4 H, and C3 N have been observed in 11 stars. We have detected the ground state 29SiO J=2−1 maser in several stars. We have also detected HCN emission in VY CMa. A narrow H13CN spike feature near the central velocity has been found in the spectrum of CRL 2688.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
10
Average
Average
Average
gold