Zobrazeno 1 - 10
of 444
pro vyhledávání: '"Kuncic Z"'
Publikováno v:
International Journal of Nanomedicine, Vol Volume 15, Pp 1253-1266 (2020)
Yaser Hadi Gholami, 1–3 Hushan Yuan, 4 Moses Q Wilks, 4 Richard Maschmeyer, 1 Marc D Normandin, 4 Lee Josephson, 4 Georges El Fakhri, 4 Zdenka Kuncic 1, 2, 5 1Faculty of Science, School of Physics, The University of Sydney, Sydney, NSW, Australia;
Externí odkaz:
https://doaj.org/article/594f6852d2cd4928b1b0fcdfa5648fba
Autor:
Gholami YH, Josephson L, Akam EA, Caravan P, Wilks MQ, Pan XZ, Maschmeyer R, Kolnick A, El Fakhri G, Normandin MD, Kuncic Z, Yuan H
Publikováno v:
International Journal of Nanomedicine, Vol Volume 15, Pp 31-47 (2020)
Yaser H Gholami, 1– 4 Lee Josephson, 3 Eman A Akam, 5 Peter Caravan, 5 Moses Q Wilks, 3 Xiang-Zuo Pan, 3, 6 Richard Maschmeyer, 1 Aleksandra Kolnick, 3, 7 Georges El Fakhri, 3 Marc D Normandin, 3 Zdenka Kuncic, 1, 4, 8 Hushan Yuan 3 1The University
Externí odkaz:
https://doaj.org/article/67d723449f6d4486be25c5ff3986cc30
Autor:
Schuemann, J., McNamara, A., Warmenhoven, J. W., Henthorn, N. T., Kirkby, K., Merchant, M. J., Ingram, S., Paganetti, H., Held, KD., Ramos-Mendez, J., Faddegon, B., Perl, J., Goodhead, D., Plante, I., Rabus, H., Nettelbeck, H., Friedland, W., Kundrat, P., Ottolenghi, A., Baiocco, G., Barbieri, S., Dingfelder, M., Incerti, S., Villagrasa, C., Bueno, M., Bernal, M. A., Guatelli, S., Sakata, D., Brown, J. M. C., Francis, Z., Kyriakou, I., Lampe, N., Ballarini, F., Ca-rante, M. P., Davidkova, M., Štepán, V., Jia, X., Cucinotta, F. A., Schulte, R., Stewart, R., Carlson, D., Galer, S., Kuncic, Z., LaCombe, S., Milligan, J., Cho, S. H., Inaniwa, T., Sato, T., Durante, M, Prise, K, McMahon, S. J.
Publikováno v:
Radiation Research, 191(1): 76-92
Our understanding of radiation induced cellular damage has greatly improved over the past decades. Despite this progress, there are still many obstacles to fully understanding how radiation interacts with biologically relevant cellular components to
Externí odkaz:
http://arxiv.org/abs/2201.11849
It has been proposed that the radio spectra of radio-quiet quasars is produced by free-free emission in the optically thin part of an accretion disc wind. An important observational constraint on this model is the observed X-ray luminosity. We invest
Externí odkaz:
http://arxiv.org/abs/1012.4741
The characteristic properties of blazars (rapid variability, strong polarization, high brightness) are widely attributed to a powerful relativistic jet oriented close to our line of sight. Despite the spectral energy distributions (SEDs) being strong
Externí odkaz:
http://arxiv.org/abs/0908.2337
In an earlier paper, we presented the first evidence for a bow-shock nebula surrounding the X-ray binary LMC X-1 on a scale of ~15 pc, which we argued was powered by a jet associated with an accretion disk. We now present the first evidence for an io
Externí odkaz:
http://arxiv.org/abs/0809.2140
Autor:
Soria, R., Kuncic, Z.
Publikováno v:
Adv.Space Res.42:517-522,2008
In the absence of direct kinematic measurements, the mass of an accreting black hole is sometimes inferred from the X-ray spectral parameters of its accretion disk; specifically, from the temperature and normalization of a disk-blackbody model fit. S
Externí odkaz:
http://arxiv.org/abs/0705.1374
Compton scattering of X-rays in the bulk flow of the accretion column in magnetic cataclysmic variables (mCVs) can significantly shift photon energies. We present Monte Carlo simulations based on a nonlinear algorithm demonstrating the effects of Com
Externí odkaz:
http://arxiv.org/abs/0704.1516
We examine the possibility that Ultraluminous X-ray sources (ULXs) represent the extreme end of the black hole X-ray binary (XRB) population. Based on their X-ray properties, we suggest that ULXs are persistently in a high/hard spectral state and we
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611040
Publikováno v:
Mon.Not.Roy.Astron.Soc.372:630-638,2006
We calculate the broadband radio--X-ray spectra predicted by microblazar and microquasar models for Ultra-Luminous X-ray sources (ULXs), exploring the possibility that their dominant power-law component is produced by a relativistic jet, even at near
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606707