Erratum: “The Role of Binarity and Stellar Rotation in the Split Main Sequence of NGC 2422” (2022, ApJ, 938, 42)
Chenyu He(Sun Yat-sen University), Zara Randriamanakoto(University of Antananarivo), Baitian Tang(Sun Yat-sen University), Zhengyi Shao(Shanghai Astronomical Observatory), Songmei Qin(Shanghai Astronomical Observatory), Jing Zhong(Shanghai Astronomical Observatory), Li Chen(Shanghai Astronomical Observatory), Lu Li(Shanghai Astronomical Observatory), Chengyuan Li(Chinese Academy of Sciences), Weijia Sun(Leibniz Institute for Astrophysics Potsdam), Richard de Grijs(Peking University)
Cited by 1
Related Papers
The first data release (DR1) of the LAMOST regular survey
|Research in Astronomy and Astrophysics|2015|853
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
ESTIMATION OF DISTANCES TO STARS WITH STELLAR PARAMETERS FROM LAMOST
|The Astronomical Journal|2015|42
THE NEAREST HIGH-VELOCITY STARS REVEALED BY LAMOST DATA RELEASE 1
|The Astrophysical Journal Letters|2014|39