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pro vyhledávání: '"Coe, M."'
Swift J0549.7-6812 is an Be/X-ray binary system (BeXRB) in the Large Magellanic Cloud (LMC) exhibiting a 6s pulse period. Like many such systems the variable X-ray emission is believed to be driven by the underlying behaviour of the mass donor Be sta
Externí odkaz:
http://arxiv.org/abs/2306.17098
Autor:
Coe, M. J., Monageng, I. M., Kennea, J. A., Buckley, D. A. H., Evans, P. A., Udalski, A., Groot, Paul, Bloemen, Steven, Vreeswijk, Paul, McBride, Vanessa, Klein-Wolt, Marc, Woudt, Patrick, Körding, Elmar, Poole, Rudolf Le, Pieterse, Danielle
SXP 15.6 is a recently established Be star X-ray binary system (BeXRB) in the Small Magellanic Cloud (SMC). Like many such systems the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. It is shown here that the
Externí odkaz:
http://arxiv.org/abs/2204.12960
We report on the discovery of Swift J011511.0-725611, a rare Be X-ray binary system (BeXRB) with a White Dwarf (WD) compact object, in the Small Magellanic Cloud (SMC) by S-CUBED, a weekly X-ray/UV survey of the SMC by the Neil Gehrels Swift Observat
Externí odkaz:
http://arxiv.org/abs/2109.05307
RX J0123.4-7321 is a well-established Be star X-ray binary system (BeXRB) in the Small Magellanic Cloud (SMC). Like many such systems the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. Previous work has shown
Externí odkaz:
http://arxiv.org/abs/2106.01231
Autor:
Coe, M. J., Kennea, J. A., Evans, P. A., Townsend, L. J., Udalski, A., Monageng, I. M., Buckley, D. A. H.
Swift J004929.5-733107 is an X-ray source in the Small Magellanic Cloud (SMC) that has been reported several times, but the optical counterpart has been unclear due to source confusion in a crowded region of the SMC. Previous works proposed [MA93] 30
Externí odkaz:
http://arxiv.org/abs/2104.02790
Autor:
Kennea, J. A., Coe, M. J., Evans, P. A., Monageng, I. M., Townsend, L. J., Siegel, M. H., Udalski, A., Buckley, D. A. H.
We report on the discovery of Swift J004516.6-734703, a Be/X-ray binary system by the Swift SMC Survey, S-CUBED. Swift J004516.6-734703, or SXP 146.6, was found to be exhibiting a bright (~10^37 erg/s) X-ray outburst in 2020 June 18. The historical U
Externí odkaz:
http://arxiv.org/abs/2006.12537
Swift J004427.3-734801 is an X-ray source in the Small Magellanic Cloud (SMC) that was first discovered as part of the Swift S-CUBED programme in January 2020. It was not detected in any of the previous 3 years worth of observations. The accurate pos
Externí odkaz:
http://arxiv.org/abs/2005.02891
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Autor:
Corbet, R. H. D., Chomiuk, L., Coe, M. J., Coley, J. B., Dubus, G., Edwards, P. G., Martin, P., McBride, V. A., Stevens, J., Strader, J., Townsend, L. J.
We report the identification from multi-wavelength observations of the Fermi Large Area Telescope (LAT) source 4FGL J1405.1-6119 (= 3FGL J1405.4-6119) as a high-mass gamma-ray binary. Observations with the LAT show that gamma-ray emission from the sy
Externí odkaz:
http://arxiv.org/abs/1908.10764