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19942009
most citedA Long Look at the Be/X-Ray Binaries of the Small Magellanic Cloud

89 citations · 499 across the 16 of their papers we have counts for

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Showing 2008 · astro-phShow all

6 papers · 2 filters

astro-ph20088 cited

Properties of X-ray Binaries in the Magellanic Clouds from RXTE and Chandra Observations

R. H. D. Corbet, M. J. Coe, K. E. McGowan +4

The X-ray binary population of the SMC is very different from that of the Milky Way consisting, with one exception, entirely of transient pulsating Be/neutron star binaries. We hav…

astro-ph200819 cited

High mass X-ray binary SXP18.3 undergoes the longest Type II outburst ever seen in the Small Magellanic Cloud

M. P. E. Schurch, M. J. Coe, J. L. Galache +6

On 30th August 2006 SXP18.3 a high mass X-ray binary (HMXB) in the Small Magellanic Cloud (SMC) with an 18.3s pulse period was observed by Rossi X-ray Timing Explorer (RXTE). The s…

astro-ph2008

Optical properties of High-Mass X-ray Binaries (HMXB) in the Small Magellanic Cloud

M. J. Coe, R. H. D. Corbet, K. E. McGowan +6

The SMC represents an exciting opportunity to observe the direct results of tidal interactions on star birth. One of the best indicators of recent star birth activity is the presen…

astro-ph200837 cited

The very massive X-ray bright binary system Wack 2134 (= WR 21a)

V. S. Niemela, R. C. Gamen, R. H. Barba +5

From the radial velocities of the N IV 4058 and He II 4686 emission lines, and the N V 4604-20 absorption lines, determined in digital spectra, we report the discovery that the X-r…

astro-ph200882 cited

Spectral distribution of Be/X-ray binaries in the Small Magellanic Cloud

V. A. McBride, M. J. Coe, I. Negueruela +2

The spectral distributions of Be/X-ray binaries in the Large Magellanic Cloud and Galaxy have been shown to differ significantly from the distribution of isolated Be stars in the G…

astro-ph200889 cited

A Long Look at the Be/X-Ray Binaries of the Small Magellanic Cloud

J. L. Galache, R. H. D. Corbet, M. J. Coe +5

We have monitored 41 Be/X-ray binary systems in the Small Magellanic Cloud over ~9 years using PCA-RXTE data from a weekly survey program. The resulting light curves were analysed…