<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 flows
Kazumine Moriyasu(Tokushima University), Weijia Sun(Leibniz Institute for Astrophysics Potsdam), Kazuhiro Sakai(Utsunomiya University)
Cited by 30
Related Papers
Physical Parameters of Late-type Contact Binaries in the Northern Catalina Sky Survey
|The Astrophysical Journal Supplement Series|2020|56
Stellar Rotation and the Extended Main-sequence Turnoff in the Open Cluster NGC 5822
|The Astrophysical Journal|2019|45
THE STAR CLUSTER MASS–GALACTOCENTRIC RADIUS RELATION: IMPLICATIONS FOR CLUSTER FORMATION
|The Astrophysical Journal|2015|13
Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. II. Statistics
|The Astrophysical Journal|2021|13
The role of tidal interactions in the formation of slowly rotating early-type stars in young star clusters
|Monthly Notices of the Royal Astronomical Society|2023|12