Zobrazeno 1 - 10
of 210
pro vyhledávání: '"Brocksopp, C."'
Autor:
Chun, Y. Y., Dinçer, T., Kalemci, E., Güver, T., Tomsick, J. A., Buxton, M. M., Brocksopp, C., Corbel, S., Cabrera-Lavers, A.
Galactic black hole transients show many interesting phenomena during outburst decays. We present simultaneous X-ray (RXTE, Swift, and INTEGRAL), and optical/near-infrared (O/NIR) observations (SMARTS) of the X-ray transient XTE J1752-223 during its
Externí odkaz:
http://arxiv.org/abs/1304.6336
Autor:
Corbel, S., Aussel, H., Broderick, J. W., Chanial, P., Coriat, M., Maury, A. J., Buxton, M., Tzioumis, J. A. Tomsick A., Markoff, S., Rodriguez, J., Bailyn, C., Brocksopp, C., Fender, R., Petrucci, P. O., Cadolle-Bel, M., Calvelo, D., Harvey-Smith, L.
Galactic black hole binaries produce powerful outflows with emit over almost the entire electromagnetic spectrum. Here, we report the first detection with the Herschel observatory of a variable far-infrared source associated with the compact jets of
Externí odkaz:
http://arxiv.org/abs/1303.2551
Autor:
Corbel, S., Coriat, M., Brocksopp, C., Tzioumis, A. K., Fender, R. P., Tomsick, J. A., Buxton, M. M., Bailyn, C. D.
The existing radio and X-ray flux correlation for Galactic black holes in the hard and quiescent states relies on a sample which is mostly dominated by two sources (GX 339-4 and V404 Cyg) observed in a single outburst. In this paper, we report on a s
Externí odkaz:
http://arxiv.org/abs/1211.1600
Spectral evolution of the X-ray nova XTE J1859+226 during its outburst observed by BeppoSAX and RXTE
Autor:
Farinelli, R., Amati, L., Shaposhnikov, N., Frontera, F., Masetti, N., Palazzi, E., Landi, R., Lombardi, C., Orlandini, M., Brocksopp, C.
We report results of an extensive analysis of the X-ray nova XTE J1859+226 observed with BeppoSAX and RXTE during its 1999 outburst. We modelled the source spectrum with a multicolour blackbody-like feature plus the generic Comptonization model BMC w
Externí odkaz:
http://arxiv.org/abs/1211.1270
The Galactic X-ray transient XTE J1752-223 was shown to have properties of black hole binary candidates. As reported in our previous paper, we identified transient and decelerating ejecta in multi-epoch Very Long Baseline Interferometry (VLBI) observ
Externí odkaz:
http://arxiv.org/abs/1108.3492
Autor:
Krimm, H. A., Tomsick, J. A., Markwardt, C. B., Brocksopp, C., Grise, F., Kaaret, P., Romano, P.
We report on the discovery by the Swift Gamma-Ray Burst Explorer of the black hole candidate Swift J1539.2-6227 and the subsequent course of an outburst beginning in November 2008 and lasting at least seven months. The source was discovered during no
Externí odkaz:
http://arxiv.org/abs/1104.4801
Autor:
Curran, P. A., Casella, P., Maccarone, T. J., Evans, P. A., Landsman, W., Krimm, H. A., Brocksopp, C., Still, M.
Here we summarise the Swift broadband observations of the recently discovered X-ray transient and black hole candidate, XTE J1752-223,obtained over the period of outburst from October 2009 to June 2010. We offer a phenomenological treatment of the sp
Externí odkaz:
http://arxiv.org/abs/1104.0796
Autor:
Miller-Jones, J. C. A., Jonker, P. G., Ratti, E. M., Torres, M. A. P., Brocksopp, C., Yang, J., Morrell, N. I.
Using high-precision astrometric optical observations from the Walter Baade Magellan Telescope in conjunction with high-resolution very long baseline interferometric (VLBI) radio imaging with the Very Long Baseline Array (VLBA), we have located the c
Externí odkaz:
http://arxiv.org/abs/1103.2826
Autor:
Coriat, M., Corbel, S., Prat, L., Miller-Jones, J. C. A., Cseh, D., Tzioumis, A. K., Brocksopp, C., Rodriguez, J., Fender, R. P., Sivakoff, G. R.
In recent years, much effort has been devoted to unraveling the connection between the accretion flow and the jets in accreting compact objects. In the present work, we report new constraints on these issues, through the long term study of the radio
Externí odkaz:
http://arxiv.org/abs/1101.5159
The recently discovered Galactic X-ray transient XTE J1752-223 entered its first known outburst in 2010, emitting from the X-ray to the radio regimes. Its general X-ray properties were consistent with those of a black hole candidate in various spectr
Externí odkaz:
http://arxiv.org/abs/1009.1367