Figure 10 from The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The ¹⁹F(α, p)²²Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars

Authors: G. D'Agata, R. G. Pizzone, M. La Cognata, I. Indelicato, C. Spitaleri, S. Palmerini, O. Trippella, D. Vescovi, S. Blagus, S. Cherubini, P. Figuera, L. Grassi, G. L. Guardo, M. Gulino, S. Hayakawa, R. Kshetri, L. Lamia, M. Lattuada, T. Mijatovic`, M. Milin, Đ. Miljanic`, L. Prepolec, G. G. Rapisarda, S. Romano, M. L. Sergi, N. Skukan, N. Soic`, V. Tokic`, A. Tumino, and M. Uroic`

2018 The Astrophysical Journal 860 61.

Provider: AAS Journals

Caption: Figure 10.

HOES cross-section for the ¹⁹F(α, p)²²Ne reaction. The blue line with the red band represents the Modified R-matrix fit along with its error (respectively, see the text for details). All the resonances used for the fit are reported in Table 2.

Other Images in This Article

Copyright and Terms & Conditions