A new r-process star with low abundances of r-process elements

6th Nuclear Physics in Astrophysics

物理学;天文学

Frebel, A.^1 ; Yu, Q.^1 ; Jacobson, H.R.^1

Department of Physics, Massachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research, Cambridge

MA

02139, United States^1

关键词: Absorption lines;    Chemical abundance;    Element abundances;    Metal-poor star;    Neutron capture;    Production sites;    Stellar spectra;    Strong enhancement;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/665/1/012051/pdf
DOI  :  10.1088/1742-6596/665/1/012051

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

Metal-poor stars with measurable r-process element abundances provide key clues to the production site(s) of the r-process and how its products are mixed with the surrounding medium. While the number of stars exhibiting strong enhancements of r-process elements has grown over the years, the lower "floor" of r-process enrichment in metal-poor stars has yet to be established, largely in part due to the difficulty in detecting weak neutron-capture element absorption lines in stellar spectra. Here we present detailed abundances of 16 neutron-capture elements for a star exhibiting the lowest level of r-process enrichment yet detected and still following the solar system r-process pattern. Taken into consideration with most of the r- process enriched stars currently in the literature, the range of r-process element enrichment spanned by this sample is at least ∼1.3dex or a factor of more than 20. That the r-process abundance pattern is unchanged while the degree of enrichment varies may suggest that the r- process yields are constant while the gas mass into which they are mixed varies. Given that all stars have similar [Fe/H] values then suggests that only one or few previous stellar generations provided the observed chemical abundances, meaning that perhaps only one r-process event occurred prior to their formation. This would be consistent with a (near) constant r-process yield per event. Obtaining detailed element abundances for stars with mild r-process element enhancements is necessary to better constrain the ubiquity of the r-process pattern, the yields of r-process elements, and the site of its production.