Published December 10, 2024
| Version v1
Dataset
Open
Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars
Contributors
Project leader (2):
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1.
Zhejiang Lab
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2.
Beijing Normal University
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3.
National Astronomical Observatories
- 4. Interdisciplinary Center for Scientific Computing
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5.
University of Hawaiʻi at Mānoa
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6.
Beijing Planetarium
Description
The dataset used in the paper "Young O-rich Stars Migrated from the Outer Disc: Imprints of Sagittarius Accretion Event".
Files
Source_data_age.csv
Additional details
Related works
- Is supplement to
- Dataset: arXiv:2311.05815 (arXiv)
Dates
- Accepted
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2024-12-10The stellar age used in the paper