Physical Parameters of Late-type Contact Binaries in the Northern Catalina Sky SurveyWeijia Sun, Richard de Grijs, Xiaodian Chen et al.|The Astrophysical Journal Supplement Series|2020Cited by 56
Stellar Rotation and the Extended Main-sequence Turnoff in the Open Cluster NGC 5822Weijia Sun, Michael D. Albrow, Richard de Grijs et al.|The Astrophysical Journal|2019Cited by 45
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:msup><mml:mrow><mml:mi>C</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msup></mml:math>-stably expansive flowsKazumine Moriyasu, Weijia Sun, Kazuhiro Sakai|Journal of Differential Equations|2004Cited by 30
THE STAR CLUSTER MASS–GALACTOCENTRIC RADIUS RELATION: IMPLICATIONS FOR CLUSTER FORMATIONWeijia Sun, Ewan Cameron, Richard de Grijs et al.|The Astrophysical Journal|2015Cited by 13
Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. II. StatisticsWeijia Sun, Richard de Grijs, Xiao-Wei Duan et al.|The Astrophysical Journal|2021Cited by 13