A λ2 mm molecular line survey of the C-star envelope IRC+10216
Astron. Astrophys. Suppl. Ser., 142 2 (2000) 181-215
Published online: 2000-03-15
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https://doi.org/10.1088/0004-637X/691/2/1660
SUBMILLIMETER NARROW EMISSION LINES FROM THE INNER ENVELOPE OF IRC+10216
Nimesh A. Patel, Ken H. Young, Sandra Brünken, et al.The Astrophysical Journal 692 (2) 1205 (2009)
https://doi.org/10.1088/0004-637X/692/2/1205
DENSITY-ENHANCED GAS AND DUST SHELLS IN A NEW CHEMICAL MODEL FOR IRC+10216
M. A. Cordiner and T. J. MillarThe Astrophysical Journal 697 (1) 68 (2009)
https://doi.org/10.1088/0004-637X/697/1/68
Circumstellar water vapour in M-type AGB stars: constraints from H$_{\sf 2}$O(1$_{\sf 10}$–1$_{\sf 01}$) lines obtained with Odin
M. Maercker, F. L. Schöier, H. Olofsson, et al.Astronomy & Astrophysics 494 (1) 243 (2009)
https://doi.org/10.1051/0004-6361:200810017
Science with the Atacama Large Millimeter Array
M. Agúndez, J. Cernicharo, J. R. Pardo, et al.Science with the Atacama Large Millimeter Array 229 (2008)
https://doi.org/10.1007/978-1-4020-6935-2_41
A Detailed Analysis of the Dust Formation Zone of IRC +10216 Derived from Mid‐Infrared Bands of C2H2and HCN
J. P. Fonfria, J. Cernicharo, M. J. Richter and J. H. LacyThe Astrophysical Journal 673 (1) 445 (2008)
https://doi.org/10.1086/523882