Zobrazeno 1 - 10
of 178
pro vyhledávání: '"Peele, Andrew"'
Autor:
Abbey, Brian, Dilanian, Ruben A., Darmanin, Connie, Ryan, Rebecca A., Putkunz, Corey T., Martin, Andrew V., Streltsov, Victor, Jones, Michael W. M., Gaffney, Naylyn, Hofmann, Felix, Williams, Garth J., Boutet, Sebastian, Messerschmidt, Marc, Siebert, M. Marvin, Williams, Sophie, Curwood, Evan, Balaur, Eugeniu, Peele, Andrew G., Nugent, Keith A., Quiney, Harry M.
X-ray Free-Electron Lasers (XFELs) deliver X-ray pulses with a coherent flux that is approximately eight orders of magnitude greater than that available from a modern third generation synchrotron source. The power density in an XFEL pulse may be so h
Externí odkaz:
http://arxiv.org/abs/1209.5168
4U2206+54 - an Unusual High Mass X-ray Binary with a 9.6 Day Orbital Period but No Strong Pulsations
Autor:
Corbet, Robin H. D., Peele, Andrew G.
Rossi X-ray Timing Explorer All-Sky Monitor observations of the X-ray source 4U2206+54, previously proposed to be a Be star system, show the X-ray flux to be modulated with a period of approximately 9.6 days. If the modulation is due to orbital varia
Externí odkaz:
http://arxiv.org/abs/astro-ph/0107131
Autor:
Corbet, Robin H. D., Peele, Andrew G.
We present the results of Rossi X-ray Timing Explorer observations of the Be star X-ray binary system RX J0812.4-3114. A light curve obtained with the RXTE All-Sky Monitor shows that the source is currently in an active state with outbursts occurring
Externí odkaz:
http://arxiv.org/abs/astro-ph/9912316
Rossi X-ray Timing Explorer (RXTE) All-Sky Monitor (ASM) observations of the X-ray binary 2S0114+650 show modulations at periods close to both the optically derived orbital period (11.591 days) and proposed pulse period (~ 2.7 hr). The pulse period s
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809216
Autor:
Corbet, Robin H. D., Peele, Andrew G.
Rossi X-ray Timing Explorer (RXTE) All Sky Monitor observations of the transient Be star X-ray source X0726-260 suggest a 34.5 day period. This is apparently confirmed by a serendipitous RXTE Proportional Counter Array (PCA) slew detection of the sou
Externí odkaz:
http://arxiv.org/abs/astro-ph/9708239
Autor:
Carroll, Aidan J, van Riessen, Grant, Balaur, Eugeniu, Dolbnya, IP, Tran, Giang N, Peele, Andrew
We present an iterative method for polychromatic phase contrast imaging that is suitable for broadband illumination and which allows for the quantitative determination of the thickness of an object given the refractive index of the sample material. E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06efba31fa5a5b20a1bcea7bcf522c70