Abstract
A 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.
References
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© 1988 Springer-Verlag
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Nguyen-Q-Rieu et al. (1988). A sensitive line search in circumstellar envelopes. In: Nomoto, K. (eds) Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion. Lecture Notes in Physics, vol 305. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0034586
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DOI: https://doi.org/10.1007/BFb0034586
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