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- W4313265373 abstract "This work presents timing and spectral analysis of 4U 2206 $$+$$ 54 using data obtained from LAXPC instrument onboard India’s AstroSat mission. This source was observed with AstroSat in September–October 2016. We report detection of 5648 (4) s pulsations at MJD 57669 in the latter observation of 4U 2206 $$+$$ 54. The pulse profile is sinusoidal and the inherent shape is independent of energy up to 30 keV. The pulse fraction increases with energy from $$sim $$ 0.5 to $$sim $$ 0.8%. We report an updated spin-down rate of $$2.95 (14) times 10^{-7}$$ s s $$^{-1}$$ . This is about 0.40 times smaller than the previously reported long term value. The energy spectrum is best modeled with an absorbed power-law with high energy exponential cut-off. We have detected presence of broad emission line in 4U 2206 $$+$$ 54 at an energy of 7 keV with equivalent width of $$sim $$ 0.4 keV." @default.
- W4313265373 created "2023-01-06" @default.
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- W4313265373 date "2022-12-19" @default.
- W4313265373 modified "2023-10-10" @default.
- W4313265373 title "Change in spin-down rate and detection of emission line in HMXB 4U 2206$$+$$54 with AstroSat observation" @default.
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- W4313265373 doi "https://doi.org/10.1007/s12036-022-09890-z" @default.
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