The origin of elements: the need for UV spectra
Thanks to the long-term collaborations between nuclear and astrophysics, we have good understanding on stellar nucleosynthesis, except for the elements around Ti and some neutron-capture elements. From the comparison between observations and Galactic chemical evolution models, it is necessary to hav...
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| Veröffentlicht in: | Experimental astronomy 2023-02, Vol.55 (1), p.75-82 |
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| creator | Kobayashi, Chiaki |
| description | Thanks to the long-term collaborations between nuclear and astrophysics, we have good understanding on stellar nucleosynthesis, except for the elements around Ti and some neutron-capture elements. From the comparison between observations and Galactic chemical evolution models, it is necessary to have the rapid neutron-capture process associated with core-collapse supernovae, although the explosion mechanism is unknown. The impact of rotating massive stars is also shown in this paper. Many of the key elements can be exclusively obtained in the UV, and therefore without UV spectra it would not be possible to fully understand the origin of elements in the universe. |
| doi_str_mv | 10.1007/s10686-022-09862-9 |
| format | Article |
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| subjects | Astronomical models Astronomy Chemical evolution Chemistry and Earth Sciences Computer Science Galactic evolution Massive stars Nuclear capture Nuclear fusion Observations and Techniques Original Article Physics Physics and Astronomy Statistics for Engineering Stellar rotation Stellar spectra Supernovae Ultraviolet spectra |
| title | The origin of elements: the need for UV spectra |
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