Insights on the Optical and Infrared Nature of MAXI J0709-159: Implications for High-Mass X-ray Binaries

In our previous study (Bhattacharyya et al., 2022), HD~54786, the optical counterpart of the MAXI J0709-159 system, was identified to be an evolved star, departing from the main sequence, based on comparisons with non-X-ray binary systems. In this paper, using color-magnitude diagram (CMD) analysis...

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Veröffentlicht in:	arXiv.org 2024-04
Hauptverfasser:	Bhattacharyya, Suman, Blesson Mathew, Banerjee, Gourav, Sindhu, G, Muneer, S, S Pramod Kumar, Joshi, Santosh
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Color-magnitude diagram Optical counterparts (astronomy) Optical properties X ray binaries X ray stars
Online-Zugang:	Volltext
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