Evolutionary implications of the new triple-α nuclear reaction rate for low mass stars (Research Note)
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Description
Context.Ogata et al. (2009, Progr. Theor. Phys., 122, 1055) presented a theoretical determination of the 4He(αα, γ)12C, or triple-α, nuclear reaction rate. Their rate differs from the NACRE rate by many orders of magnitude at temperatures relevant for
| Collections | ANU Research Publications |
|---|---|
| Date published: | 2009 |
| Type: | Journal article |
| URI: | http://hdl.handle.net/1885/80276 |
| Source: | Astronomy and Astrophysics |
| DOI: | 10.1051/0004-6361/200912998 |
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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Dotter_Evolutionary_implications_of_2009.pdf | 220.12 kB | Adobe PDF | Request a copy |
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