The Secondary Component of the Extremely Low Mass Ratio Massive Binary HD 165246 Revealed by GHOST
C. N. Rodriguez, T. Ansin,G. A. Ferrero, O. G. Benvenuto, R. Gamen,N. I. Morrell,J. I. Arias, R. E. Higa,C. Putkuri, C. Johnston, K. Chiboucas, E. Deibert, C. R. Hayes, J.-E. Heo, M. Jeong, V. Kalari,E. Martioli,V. M. Placco,K. A. Venn, S. Xu, R. Diaz, M. Gomez-Jimenez, R. Ruiz-Carmona, C. Simpson,A. W. McConnachie,J. Pazder,G. Burley,T. A. M. Berg, J. G. Robertson,K. Labrie, J. Thomas-Osip The Astrophysical Journal（2025）
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Massive stars,Early-type stars,Fundamental parameters of stars,Close binary stars,Eclipsing binary stars
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