Zobrazeno 1 - 10
of 1 108
pro vyhledávání: '"Vaughan B"'
Publikováno v:
International Journal of Nanomedicine, Vol Volume 14, Pp 2191-2206 (2019)
Susan Hua,1,2 Benjamin Vaughan3 1Therapeutic Targeting Research Group, School of Biomedical Sciences and Pharmacy, University of Newcastle, Callaghan, NSW, Australia; 2Hunter Medical Research Institute, New Lambton Heights, NSW, Australia; 3Centre fo
Externí odkaz:
https://doaj.org/article/d08b6b390bde4393b7912acd288791f0
Autor:
McLean, D., Cure, K., Abdul Wahab, M.A., Galaiduk, R., Birt, M., Vaughan, B., Colquhoun, J., Case, M., Radford, B., Stowar, M., Harries, S., Heyward, A., Miller, K.
Publikováno v:
In Continental Shelf Research 15 April 2021 219
Autor:
Baker, Vaughan B.
Publikováno v:
Louisiana History: The Journal of the Louisiana Historical Association, 2007 Jul 01. 48(3), 261-272.
Externí odkaz:
https://www.jstor.org/stable/4234283
Autor:
Mendez, M., van der Klis, M., van Paradijs, J., Lewin, W. H. G., Vaughan, B. A., Kuulkers, E., Zhang, W., Lamb, F. K., Psaltis, D.
Using a new technique to improve the sensitivity to weak Quasi-Periodic Oscillations (QPO) we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~ 600-900 Hz peak previously reporte
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712140
There have been a number of recent spectral models that have been successful in reproducing the observed X-ray spectra of galactic black hole candidates (GBHC). However, there still exists controversy over such issues as: what are the sources of hard
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712106
Autor:
Mendez, M., van der Klis, M., van Paradijs, J., Lewin, W. H. G., Vaughan, B. A., Kuulkers, E., Zhang, W., Lamb, F. K., Psaltis, D.
Using a new technique to improve the sensitivity to weak Quasi-Periodic Oscillations (QPO) we discovered a new QPO peak at about 1100 Hz in the March 1996 outburst observations of 4U 1608-52, simultaneous with the ~ 600-900 Hz peak previously reporte
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712085
Autor:
Mendez, M., van der Klis, M., van Paradijs, J., Lewin, W. H. G., Lamb, F. K., Vaughan, B. A., Kuulkers, E., Psaltis, D.
We report three RXTE/PCA observations of the low-mass X-ray binary 4U 0614+09. They show strong (~ 30% rms) band-limited noise with a cut-off frequency varying between 0.7 and 15 Hz in correlation with the X-ray flux. We observe two non-simultaneous
Externí odkaz:
http://arxiv.org/abs/astro-ph/9705250
Autor:
Baker, Vaughan B.
Publikováno v:
Louisiana History: The Journal of the Louisiana Historical Association, 2001 Jul 01. 42(3), 261-275.
Externí odkaz:
https://www.jstor.org/stable/4233759
Autor:
Berger, M., van der Klis, M., van Paradijs, J., Lewin, W. H. G., Lamb, F., Vaughan, B., Kuulkers, E., Augusteijn, T., Zhang, W., Marshall, F. E., Swank, J. H., Lapidus, I., Lochner, J. C., Strohmayer, T. E.
We present results of RXTE observations of the low-mass X-ray binary and atoll source 4U 1608$-$52 made over 9 days during the decline of an X-ray intensity outburst in March 1996. A fast-timing analysis shows a strong and narrow quasi periodic oscil
Externí odkaz:
http://arxiv.org/abs/astro-ph/9607110
Autor:
Van der Klis, M., Swank, J. H., Zhang, W., Jahoda, K., Morgan, E. H., Lewin, W. H. G., Vaughan, B., Van Paradijs, J.
We report the discovery, with NASA's Rossi X-ray Timing Explorer (RXTE), of the first sub-millisecond oscillation found in a celestial X-ray source. The quasi-periodic oscillations (QPO) come from Sco X-1 and have a frequency of approximately 1100 Hz
Externí odkaz:
http://arxiv.org/abs/astro-ph/9607047