424 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Peking UniversityCN65 papers
- Kavli Institute for Theoretical SciencesCN31 papers
- Chinese Academy of SciencesCN16 papers
- National Astronomical ObservatoriesCN12 papers
- University of Science and Technology of ChinaCN10 papers
- Institute of High Energy PhysicsCN8 papers
- Centre National de la Recherche ScientifiqueFR7 papers
- Budker Institute of Nuclear PhysicsRU6 papers
- Institute of Modern PhysicsCN6 papers
- Novosibirsk State UniversityRU6 papers
- Ruhr University BochumDE6 papers
- Siberian Branch of the Russian Academy of SciencesRU6 papers
6 papers · 1 filter
Ba-enhanced dwarf and subgiant stars in the LAMOST Galactic surveys
Meng Zhang, Maosheng Xiang, Hua-Wei Zhang +3
Ba-enhanced stars are interesting probes of stellar astrophysics and Galactic formation history. In this work, we investigate the chemistry and kinematics for a large sample of Ba-…
Li-rich Giants in LAMOST Survey. III. The statistical analysis of Li-rich giants
Yutao Zhou, Chun Wang, Hongliang Yan +5
The puzzle of Li-rich giant is still unsolved, contradicting the prediction of the standard stellar models. Although the exact evolutionary stages play a key role in the knowledge…
Dynamical Effects of Colliding Outflows in Binary Systems
Lile Wang, Xinyu Li
The outflow of an object traveling in a fluid can shape the fluid morphology by forming a forward bow shock which accelerates the object via gravitational feedback. This dynamical…
MagAO observations of the binary microlens OGLE-2014-BLG-1050 prefer the higher-mass solution
Xiaojia Xie, Subo Dong, Wei Zhu +9
We report adaptive-optics (AO) follow-up imaging of OGLE-2014-BLG-1050, which is the second binary microlensing event with space-based parallax measurements. The degeneracy in micr…
The spatial distributions of blue main-sequence stars in Magellanic Cloud star clusters
Yujiao Yang, Chengyuan Li, Richard de Grijs +1
The color-magnitude diagrams (CMDs) of young star clusters show that, particularly at ultraviolet wavelengths, their upper main sequences (MSs) bifurcate into a sequence comprising…
The Eruption of the Candidate Young Star ASASSN-15qi
Gregory J. Herczeg, Subo Dong, Benjamin J. Shappee +27
Outbursts on young stars are usually interpreted as accretion bursts caused by instabilities in the disk or the star-disk connection. However, some protostellar outbursts may not f…