The Secondary Component of the Extremely Low Mass Ratio Massive Binary HD 165246 Revealed by GHOST

The Secondary Component of the Extremely Low Mass Ratio Massive Binary HD 165246 Revealed by GHOST

In the pursuit of understanding the multiplicity of massive stars, the OWN Survey has undertaken spectroscopic monitoring of hundreds of targets over the past 20 yr. This effort has led to the discovery of new single-lined spectroscopic binaries. Characterizing the unseen companions of these systems...

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Main Authors: 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
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Massive stars
Early-type stars
Fundamental parameters of stars
Close binary stars
Eclipsing binary stars
Online Access:https://doi.org/10.3847/1538-4357/ada892
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https://doi.org/10.3847/1538-4357/ada892

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