A Precessing Stellar Disk Model for Superorbital Modulations of the Gamma-Ray Binary LS I+61° 303

被引:1
作者
Chen, A. M. [1 ,2 ]
Takata, J. [3 ]
Yu, Y. W. [2 ,4 ]
机构
[1] Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 201210, Peoples R China
[2] Cent China Normal Univ, MOE, Key Lab Quark & Lepton Phys, Wuhan 430079, Peoples R China
[3] Huazhong Univ Sci & Technol, Sch Phys, Dept Astron, Wuhan 430074, Peoples R China
[4] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
基金
国家重点研发计划; 中国博士后科学基金; 中国国家自然科学基金;
关键词
HIGH-ENERGY EMISSIONS; LONG-TERM MODULATION; X-RAY; VERITAS OBSERVATIONS; ORBITAL PERIODS; RADIO-EMISSION; LIGHT CURVES; PULSAR WIND; H-ALPHA; VARIABILITY;
D O I
10.3847/1538-4357/ad6b0a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Gamma-ray binary LS I+61 degrees 303 consists of a neutron star orbiting around a Be star with a period of P orb similar or equal to 26.5 days. Apart from orbital modulations, the binary shows long-term flux variations with a superorbital period of Psup similar or equal to 4.6yr as seen in nearly all wavelengths. The origin of this superorbital modulation is still not well understood. Under the pulsar wind-stellar outflow interaction scenario, we propose that the superorbital modulations of LS I+61 degrees 303 could be caused by the precession of the Be disk. Assuming X-rays arise from synchrotron radiation of the intrabinary shock, we develop an analytical model to calculate expected flux modulations over the orbital and superorbital phases. The asymmetric two-peak profiles in orbital light curves and sinusoidal-like long-term modulations are reproduced under the precessing disk scenario. The observed orbital phase drifting of the X-ray peak and our fitting of long-term X-ray data indicate that the neutron star is likely orbiting around the star with a small eccentricity and periastron phase around Phi p similar to 0.6. We compare the Corbet diagrams of LS I+61 degrees 303 with other Be/X-ray binaries, and the linear correlation in the Psup-Porb diagram suggests that the precession of the Be disk in LS I+61 degrees 303 is induced by the tidal torque of its neutron star companion.
引用
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页数:11
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