Research

Identifying the Galactic Substructures in 5D Space Using All-sky RR Lyrae Stars in Gaia DR3

Date:2024-09-11

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Title:Identifying the Galactic Substructures in 5D Space Using All-sky RR Lyrae Stars in Gaia DR3

Time:Friday, September 13, 2024, 12:00 am

Speaker:Shenglan Sun (PKU)

Address:Physics Building E225

主讲人 Shenglan Sun (PKU) 时间 Friday, September 13, 2024, 12:00 am
地点 Physics Building E225 报告语言
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Motivated by the vast gap between photometric and spectroscopic data volumes, there is great potential in using 5D kinematic information to identify and study substructures of the Milky Way. We identify substructures in the Galactic halo using 46,575 RR Lyrae stars (RRLs) from Gaia DR3 with the photometric metallicities and distances newly estimated by Li et al. (2023). Assuming a Gaussian prior distribution of radial velocity, we calculate the orbital distribution characterized by the integrals of motion for each RRL based on its 3D positions, proper motions and corresponding errors, and then apply the friends-of-friends algorithm to identify groups moving along similar orbits. We find that about 28% of the sample associated with substructures, including several known substructures, such as Sagittarius (Sgr) Stream, Hercules-Aquila Cloud (HAC), Virgo Overdensity (VOD), Gaia-Enceladus-Sausage (GES), Orphan-Chenab stream, Cetus-Palca, Helmi Streams, Sequoia and Wukong, and 18 unknown groups. Our findings indicate that HAC and VOD have kinematic and chemical properties remarkably similar to GES, with ~57% of HAC and ~87% of VOD members exhibiting eccentricity as high as GES, suggesting that they may share a common origin with GES. The ability to identify the low mass and spatially dispersed substructures with radial velocity priors further demonstrates the potential of our method, which breaks the limit of spectroscopic survey and is competent to probe the substructures in the whole Galaxy. Finally, we have also identified 18 unknown groups with good spatial clustering and proper motion consistency, suggesting more excavation of MW substructures in the future with only 5D data.


BIO

Shenglan Sun is a second-year doctoral candidate in the Department of Astronomy at Peking University (PKU). Under the primary supervision of Professor Huawei Zhang, she focuses on Galactic substructure research. Her work is co-advised by Professors Yang Huang and Xiangxiang Xue from the National Astronomical Observatories of China (NAOC).


Host: Shuo Zhang

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