Chemical evidence shows how a dwarf galaxy contributes to growth of the Milky Way

Chemical evidence shows how a dwarf galaxy contributes to growth of Milky Way
Star accreted from a disrupted dwarf galaxy. Credit: Chinese National Astronomy

Small stellar systems like dwarf galaxies are thought to be the main building blocks of the Milky Way. However, it is unclear how many and what kind of stars in our galaxy originated from satellite dwarf galaxies.

An international team led by Zhao Gang, a professor from the National Astronomical Observatories of Chinese Academy of Sciences (NAOC) discovered a chemically peculiar star accreted from a disrupted dwarf galaxy. According to results obtained through the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and Subaru telescope, the star has an unusually low amount of magnesium, the eighth most in the universe. Meanwhile, it contains an excessive amount of heavy elements such as europium, gold, and uranium. The team reported their findings online in Nature Astronomy on April 29th, 2019.

"Stars preserve information of their birth sites. We can distinguish formed in the Milky Way from stars formed in based on their chemical abundances," says Zhao, who is also the corresponding author of the paper.

The chemical composition of this peculiar star suggests it originated from a dwarf galaxy that was disrupted by interaction with the Milky Way. The data was obtained by LAMOST, a spectroscopic survey telescope that takes 4,000 spectra in a single exposure. So far, LAMOST has obtained more than 8 million stellar spectra for studies of the formation of the Milky Way.

"The massive spectra provided by the LAMOST survey give us a great opportunity to find chemically peculiar stars," says Xing Qianfan, Ph.D., first author of the paper. This type of star can be used to explore the chemical evolution of stellar systems. Xing says, "This newly discovered star with large excesses of heavy elements provides a window for exploring the chemical evolution of disrupted dwarf . The in dwarf galaxies is relatively slow comparing to larger galaxies, leading to chemical differences among their stellar populations. For instance, the magnesium to iron (Mg/Fe) abundance ratios in stars of dwarf galaxies currently found around the Milky Way are much smaller than those in the majority of stars in the Milky Way."

"This is the first discovery of a star having a very low amount of magnesium and an excessive amount of heavy elements," says co-author Li Haining, Ph.D.

The extreme enhancement of heavy elements of this star suggests this dwarf galaxy was affected by high-yield rapid neutron-capture process (r-process), the dominant process through which elements heavier than iron are formed. Such process may happen during mergers of binary neutron stars in the dwarf galaxy.

"The discovery of this chemically peculiar star is a good start of chemical identification of stars accreted from dwarf galaxies. Such stars will be good tracers for exploring the assembly history of the Milky Way," says Zhao.

More information: Evidence for the accretion origin of halo stars with an extreme r-process enhancement, Nature Astronomy (2019). DOI: 10.1038/s41550-019-0764-5 ,

Journal information: Nature Astronomy

Citation: Chemical evidence shows how a dwarf galaxy contributes to growth of the Milky Way (2019, April 30) retrieved 9 December 2023 from
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