Ultra-high-resolution observations of circumstellar K I and C2 around the post-AGB star HD 56126
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/311/2/370/2878166/311-2-370.pdf
Reference22 articles.
1. First results from the UHRF: ultra-high-resolution observations of atomic interstellar lines towards ζ Ophiuchi
2. The Circumstellar Shell of the Post–Asymptotic Giant Branch Star HD 56126: The12CN/13CN Isotope Ratio and Fractionation
3. The Circumstellar Shell of the Post–Asymptotic Giant Branch Star HD 56126:12C12C/12C13C Isotope Ratio and12C16O Column Density
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1. The chemical composition of the post-asymptotic giant branch F supergiant CRL 2688;Monthly Notices of the Royal Astronomical Society;2012-08-10
2. Kinematic structure of the atmosphere and envelope of the post-AGB star HD 56126;Astronomy Reports;2007-12
3. Optical spectrum of the post-AGB Star HD56126 in the wavelength interval 4010-8790 Å Å;Astrophysical Bulletin;2007-06
4. Theoretical study on HNC(1Σ) production from the C2(X1Σg+)+NH(X3Σ-) reaction;Chemical Physics Letters;2006-10
5. Reaction dynamics of carbon-bearing radicals in circumstellar envelopes of carbon stars;Faraday Discussions;2006
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