Abstract
At this point of the study, we have been able to confirm some of the astrophysical hypotheses presented above. However, before drawing any conclusion, other determining processes such as b3, c, d1 and d2, have to be studied. This is our project.
This is a preview of subscription content, log in via an institution to check access.
References
W.M. Irvine and F.P. Schloerb, ApJ, 282, 516–521 (1984)
P. Schilke, C.M. Walmsley, G. Pineau des Forests, E. Roueff, D.R. Flower and S. Guilloteau (1992) A & A, 256, 595–612 (1992)
A. Dalgarno, F. Masnou-Seeuws, and R.W.P. McWhirter “Atomic and molecular processes in Astrophysics” (Swiss Society of Astronomy and Astrophysic, Saas-Fee 5th advanced course) (1975)
D. Talbi and Y. Ellinger, to be submitted
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1995 Springer-Verlag
About this paper
Cite this paper
Talbi, D. (1995). Around the HCNH+ chemistry astrophysical implication. In: Winnewisser, G., Pelz, G.C. (eds) The Physics and Chemistry of Interstellar Molecular Clouds. Lecture Notes in Physics, vol 459. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102143
Download citation
DOI: https://doi.org/10.1007/BFb0102143
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-60482-2
Online ISBN: 978-3-540-47665-8
eBook Packages: Springer Book Archive