086190
收藏Mendeley Data2024-01-31 更新2024-06-28 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/086190.html
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In a recent survey by combining photometry of ASAS-SN and spectroscopy of LAMOST comma a sample black hole binary candidates were selected. We speculate that they are X-ray binary systems in the quiescent state. To distinguish them from chromospherically active binaries comma we propose to use XMM-Newton observations to search for their X-ray counterparts. By measuring the X-ray spectrum and X-ray flux comma we can select the most promising black hole candidates for follow-up observations.
创建时间：
2024-01-31
