Off the wire
China sees more inclusive finance loans to small businesses in 2019  • Discover China: Digital technologies enable inclusive finance in China  • Inclusive finance service benefits small enterprises  • China inclusive finance loans increase in 2018  • China allocates 10 bln yuan to support inclusive finance  • China's inclusive finance develops steadily  • Xinhua China news advisory -- June 3  • Garden festival kicks off in Ireland, attracts residents, visitors  • Venezuela sends aid to Cuba after tropical storm Alberto  • Venezuela prepares list of political opponents to be freed from jail  
You are here:   News/

Chinese astronomers discover nearly 600 high-velocity stars

Xinhua,December 28, 2020 Adjust font size:

BEIJING, Dec. 27 (Xinhua) -- A Chinese research team has discovered 591 high-velocity stars based on data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and the European Space Agency's Gaia satellite.


High-velocity stars are stars that move unusually quickly, relative to other stars, and may at some point leave their galaxy. Of the newly discovered stars, 43 may escape the gravitational constraints of the Milky Way galaxy in future and fly into intergalactic space.


A total of over 550 high-velocity stars had been found since the first one was discovered in 2005. The new discovery has doubled the total number known, said Li Yinbi with the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), lead author of the research.


High-velocity stars can provide deep insights into a wide range of topics within galactic science, from the central supermassive black hole to the distant galactic halo, according to Lu Youjun, a researcher at the NAOC.


The researchers analyzed the chemical and kinematic properties of the 591 high-speed stars and found that they are inner-halo stars. "Their low metallicities indicate that the bulk of the stellar halo formed as a consequence of the accretion and tidal disruption of dwarf galaxies," said Zhao Gang, also a researcher at the NAOC.


The discovery was recently published in the Astrophysical Journal Supplement Series.