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- W2321978497 abstract "Abstract An anti-correlation between the optical brightness and the strength of the Hα emission was observed from two Be/X-ray binaries, A0535+26 and MXB 0656-072: when the optical brightness showed a decrease, the intensity of the Hα emission displayed an obvious increase. This anti-correlation is interpreted as the result of the mass ejection from the Be star. After the mass ejection event, a cavity or low-density region will be developing in the inner parter of the circumstellar disk. The X-ray outbursts of the Be/X-ray binaries might be connected with the mass ejections from the Be star." @default.
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- W2321978497 date "2012-08-01" @default.
- W2321978497 modified "2023-10-05" @default.
- W2321978497 title "Multi-wavelength Study of the Be/X-ray Binaries" @default.
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- W2321978497 doi "https://doi.org/10.1017/s1743921312020364" @default.
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