Related references
Note: Only part of the references are listed.Water in IRC+10216: a genuine formation process by shock-induced chemistry in the inner wind
I. Cherchneff
ASTRONOMY & ASTROPHYSICS (2011)
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NATURE (2010)
DENSITY-ENHANCED GAS AND DUST SHELLS IN A NEW CHEMICAL MODEL FOR IRC+10216
M. A. Cordiner et al.
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Molecular shells in IRC+10216: Evidence for nonisotropic and episodic mass-loss enhancement
Dinh-V-Trung et al.
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The variable mass loss of the AGB star WX Piscium as traced by the CO J=1-0 through 7-6 lines and the dust emission
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The carbon star IRC+10216:: linking the complex inner region with its spherical large-scale structures
J. -L. Menut et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
Inverse Compton emission from Galactic supernova remnants: Effect of the interstellar radiation field
Troy A. Porter et al.
ASTROPHYSICAL JOURNAL (2006)
The circumstellar envelope of IRC+10216 from milli-arcsecond to arcmin scales
I. C. Leao et al.
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Properties of detached shells around carbon stars -: Evidence of interacting winds
FL Schöier et al.
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The magnetic field around late-type stars revealed by the circumstellar H2O masers
WHT Vlemmings et al.
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Three-component modeling of C-rich AGB star winds - III. Micro-physics of drift-dependent dust formation
C Sandin et al.
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Discovery of multiple molecular shells in the outer envelope of IRC+10216
D Fong et al.
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Bispectrum speckle interferometry of IRC+10216:: The dynamic evolution of the innermost circumstellar environment from 1995 to 2001
G Weigelt et al.
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Late AGB magnetic cycles:: Magnetohydrodynamic solutions for the Hubble Space Telescope planetary nebula rings
G García-Segura et al.
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Origin of quasi-periodic shells in dust forming AGB winds
YJW Simis et al.
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A solar-like cycle in asymptotic giant branch stars
N Soker
ASTROPHYSICAL JOURNAL (2000)