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21“... strongly suggest it is a binary star, we find evidence that the fainter star may be a background star...”
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22“... strongly suggest it is a binary star, we find evidence that the fainter star may be a background star...”
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23“... strongly suggest it is a binary star, we find evidence that the fainter star may be a background star...”
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24“... stars, while planets with M sin i <~ 4 M_J are less eccentric than binary stars and more massive planets...”
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25“... with that of binary stars, while planets with M sin i�4 MJ are less eccentric than binary stars and more massive...”
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26“... stars, while planets with M sin i <~ 4 M_J are less eccentric than binary stars and more massive planets...”
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27“...5. Searching for Tatooine (Planets orbiting binary stars) 6. Tracing the dust around nearby, sun...”
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28Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometryby kok, Yitping, Ireland, Michael, Rizzuto, A C, Tuthill, Peter G, Robertson, James G, Warrington, Benjamin A, Tango, W J“..., the narrow-angle astrometry of several closed binary stars (with separation less than 2″), as described...”
Published 2015
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29Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometryby Kok, Yitping, Ireland, Michael J., Rizzuto, Aaron C., Tuthill, Peter G., Robertson, J. Gordon, Warrington, Benjamin A., Tango, William J.“..., the narrow-angle astrometry of several closed binary stars (with separation less than 2″), as described...”
Published in SPIE Proceedings, Optical and Infrared Interferometry IV (2014)
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30Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometryby kok, Yitping, Rizzuto, Aaron C., Tuthill, Peter G, Robertson, James G, Warrington, Benjamin A, Tango, W J, Ireland, Michael“..., the narrow-angle astrometry of several closed binary stars (with separation less than 2″), as described...”
Published in SPIE Proceedings, Optical and Infrared Interferometry IV
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31Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometryby Kok, Y., Ireland, M. J., Rizzuto, A. C., Tuthill, P. G., Robertson, J. G., Warrington, B. A., Tango, W. J.“..., the narrow-angle astrometry of several closed binary stars (with separation less than 2$"$), as described...”
Published 2014
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32Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometryby Kok, Y., Ireland, M. J., Rizzuto, A. C., Tuthill, P. G., Robertson, J. G., Warrington, B. A., Tango, W. J.“..., the narrow-angle astrometry of several closed binary stars (with separation less than 2$"$), as described...”
Published in SPIE Proceedings, Optical and Infrared Interferometry IV (2014)
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33by Shi, Xiang-Dong, Qian, Sheng-Bang, Zhang, Jia, Soonthornthum, Boonrucksar, Sarotsakulchai, Thawicharat, Zhou, Xiao“... for the three contact binary stars. The results showed that the period of AST19571 is increasing at a rate of dp...”
Published in New Astronomy (2019)
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34by Shi XD(施相东), Qian SB(钱声帮), Zhang J(张嘉), Soonthornthum, Boonrucksar, Sarotsakulchai, Thawicharat, Zhou X(周肖)“... for the three contact binary stars. The results showed that the period of AST19571 is increasing at a rate of dp...”
Published in New Astronomy (2019)
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