Zobrazeno 1 - 10
of 152
pro vyhledávání: '"Schurch, M."'
Autor:
Fender, R., Woudt, P. A., Armstrong, R., Groot, P., McBride, V., Miller-Jones, J., Mooley, K., Stappers, B., Wijers, R., Bietenholz, M., Blyth, S., Bottcher, M., Buckley, D., Charles, P., Chomiuk, L., Coppejans, D., Corbel, S., Coriat, M., Daigne, F., de Blok, W. J. G., Falcke, H., Girard, J., Heywood, I., Horesh, A., Horrell, J., Jonker, P., Joseph, T., Kamble, A., Knigge, C., Koerding, E., Kotze, M., Kouveliotou, C., Lynch, C., Maccarone, T., Meintjes, P., Migliari, S., Murphy, T., Nagayama, T., Nelemans, G., Nicholson, G., O'Brien, T., Oodendaal, A., Oozeer, N., Osborne, J., Perez-Torres, M., Ratcliffe, S., Ribeiro, V., Rol, E., Rushton, A., Scaife, A., Schurch, M., Sivakoff, G., Staley, T., Steeghs, D., Stewart, I., Swinbank, J., van der Heyden, K., van der Horst, A., van Soelen, B., Vergani, S., Warner, B., Wiersema, K.
ThunderKAT is the image-plane transients programme for MeerKAT. The goal as outlined in 2010, and still today, is to find, identify and understand high-energy astrophysical processes via their radio emission (often in concert with observations at oth
Externí odkaz:
http://arxiv.org/abs/1711.04132
Autor:
Gonzalez-Galan, A., Oskinova, L. M., Popov, S. B., Haberl, F., Kuehnel, M., Gallagher III, J. S., Schurch, M. P. E., Guerrero, M. A.
SXP 1062 is a Be X-ray binary located in the Small Magellanic Cloud. It hosts a long-period X-ray pulsar and is likely associated with the supernova remnant MCSNR J0127-7332. In this work we present a multi-wavelength view on SXP 1062 in different lu
Externí odkaz:
http://arxiv.org/abs/1706.05002
Autor:
McBride, V. A., Gonzalez-Galan, A., Bird, A. J., Coe, M. J., Bartlett, E. S., Dorda, R., Haberl, F., Marco, A., Negueruela, I., Schurch, M. P. E., Sturm, R., Buckley, D. A. H., Udalski, A.
The X-ray binary population of the Small Magellanic Cloud (SMC) contains a large number of massive X-ray binaries and the recent survey of the SMC by XMM-Newton has resulted in almost 50 more tentative high mass X-ray binary candidates. Using probabi
Externí odkaz:
http://arxiv.org/abs/1701.05765
Autor:
Rajoelimanana, A. F., Charles, P. A., Meintjes, P. J., Townsend, L. J., Schurch, M. P. E., Udalski, A.
We combine the decade long photometry of the Be/X-ray binary system A0538-66 provided by the MACHO and OGLE IV projects with high resolution SALT spectroscopy to provide detailed constraints on the orbital parameters and system properties. The ~420d
Externí odkaz:
http://arxiv.org/abs/1609.09811
Autor:
Coppejans, D. L., Woudt, P. A., Warner, B., Koerding, E., Macfarlane, S. A., Schurch, M. P. E., Kotze, M. M., Breytenbach, H. B., Gulbis, A. A. S., Coppejans, R.
Time series photometry of 20 Cataclysmic Variables detected by the Catalina Real-time Transient Survey is presented. 14 of these systems have not been observed previously and only two have been examined in-depth. From the observations we determined 1
Externí odkaz:
http://arxiv.org/abs/1310.3642
Autor:
Armstrong, R. P., Fender, R. P., Nicolson, G. D., Ratcliffe, S., Linares, M., Horrell, J., Richter, L., Schurch, M. P. E., Coriat, M., Woudt, P., Jonas, J., Booth, R., Fanaroff, B.
Circinus X-1 is a bright and highly variable X-ray binary which displays strong and rapid evolution in all wavebands. Radio flaring, associated with the production of a relativistic jet, occurs periodically on a ~17-day timescale. A longer-term envel
Externí odkaz:
http://arxiv.org/abs/1305.3399
Autor:
Sturm, R., Haberl, F., Oskinova, L. M., Schurch, M. P. E., Hénault-Brunet, V., Gallagher III, J. S., Udalski, A.
The Be/X-ray binary SXP1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretio
Externí odkaz:
http://arxiv.org/abs/1304.6022
Autor:
Schurch, M. P. E., Coe, M. J., McBride, V. A., Townsend, L. J., Udalski, A., Haberl, F., Corbet, R. H. D.
We present an optical and X-ray study of four Be/X-ray binaries located in the Small Magellanic Cloud (SMC). OGLE I-band data of up to 11 years of semi-continuous monitoring has been analysed for SMC X-2, SXP172 and SXP202B, providing both a measurem
Externí odkaz:
http://arxiv.org/abs/1010.5621
Autor:
Townsend, L. J., Coe, M. J., Corbet, R. H. D., McBride, V. A., Hill, A. B., Bird, A. J., Schurch, M. P. E., Haberl, F., Sturm, R., Pathak, D., van Soelen, B., Bartlett, E. S., Drave, S. P., Udalski, A.
We present X-ray and optical data on the Be/X-ray binary (BeXRB) pulsar IGR J01054-7253 = SXP11.5 in the Small Magellanic Cloud (SMC). Rossi X-ray Timing Explorer (RXTE) observations of this source in a large X-ray outburst reveal an 11.483 +/- 0.002
Externí odkaz:
http://arxiv.org/abs/1008.3361
Autor:
Coe, M. J., Bird, A. J., Buckley, D. A. H., Corbet, R. H. D., Dean, A. J., Finger, M., Galache, J. L., Haberl, F., McBride, V. A., Negueruela, I., Schurch, M., Townsend, L. J., Udalski, A., Wilms, J., Zezas, A.
Deep observations of the Small Magellanic Cloud (SMC) and region were carried out in the hard X-ray band by the INTEGRAL observatory in 2008-2009. The field of view of the instrument permitted simultaneous coverage of the entire SMC and the eastern e
Externí odkaz:
http://arxiv.org/abs/1004.2219