Zobrazeno 1 - 10
of 637
pro vyhledávání: '"O’Byrne, J"'
Publikováno v:
Malaysian Orthopaedic Journal, Vol 16, Iss 2, Pp 46-54 (2022)
INTRODUCTION: COVID-19 has had a significant impact on healthcare. It has forced orthopaedic surgeons to limit face- to-face patient contact. This resulted in the ad hoc creation of a virtual arthroplasty clinic (VAC) in Irish National Orthopaedic Ho
Externí odkaz:
https://doaj.org/article/3f7be7d4759243979399dd5d5c4a1a77
Publikováno v:
In Journal of Orthopaedics January-February 2021 23:8-12
New multi-core imaging fibre bundles -- hexabundles -- being developed at the University of Sydney will provide simultaneous integral field spectroscopy for hundreds of celestial sources across a wide angular field. These are a natural progression fr
Externí odkaz:
http://arxiv.org/abs/1104.0985
Autor:
Tango, W. J., Davis, J., Jacob, A. P., Mendez, A., North, J. R., O'Byrne, J. W., Seneta, E. B., Tuthill, P. G.
The binary star delta Sco (HD143275) underwent remarkable brightening in the visible in 2000, and continues to be irregularly variable. The system was observed with the Sydney University Stellar Interferometer (SUSI) in 1999, 2000, 2001, 2006 and 200
Externí odkaz:
http://arxiv.org/abs/0811.4004
Autor:
North, J. R., Davis, J., Robertson, J. G., Bedding, T. R., Bruntt, H., Ireland, M. J., Jacob, A. P., Lacour, S., O'Byrne, J. W., Owens, S. M., Stello, D., Tango, W. J., Tuthill, P. G.
We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of the F9 V star beta Virginis. After correcting for limb darkening and combining with the revised Hipparcos parallax, we derive a radius of 1.703 +/- 0.
Externí odkaz:
http://arxiv.org/abs/0811.1804
Autor:
Davis, J., Ireland, M. J., Chow, J., Jacob, A. P., Lucas, R. E., North, J. R., O'Byrne, J. W., Owens, S. M., Robertson, J. G., Seneta, E., Tango, W. J., Tuthill, P. G.
A new beam-combination and detection system has been installed in the Sydney University Stellar Interferometer working at the red end of the visual spectrum (wavelength range 500-950 nm) to complement the existing blue-sensitive system (wavelength ra
Externí odkaz:
http://arxiv.org/abs/0709.3872
Autor:
North, J. R., Davis, J., Bedding, T. R., Ireland, M. J., Jacob, A. P., O'Byrne, J., Owens, S. M., Robertson, J. G., Tango, W. J., Tuthill, P. G.
We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of beta Hydri. This star is a nearby G2 subgiant whose mean density was recently measured with high precision using asteroseismology. We determine the ra
Externí odkaz:
http://arxiv.org/abs/0707.0333
Autor:
Davis, J., Mendez, A., Seneta, E. B., Tango, W. J., Booth, A. J., O'Byrne, J. W., Thorvaldson, E. D., Ausseloos, M., Aerts, C., Uytterhoeven, K.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 356 (2005) 1362-1370
The bright southern binary star beta Centauri (HR 5267) has been observed with the Sydney University Stellar Interferometer (SUSI) and spectroscopically with the ESO CAT and Swiss Euler telescopes at La Silla. The interferometric observations have co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411054
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Akademický článek
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