scholarly journals On the magnetic fields of Be/X-ray pulsars in the Small Magellanic Cloud: Figure 1.

2015 ◽  
Vol 454 (4) ◽  
pp. 3760-3765 ◽  
Author(s):  
N. R. Ikhsanov ◽  
S. Mereghetti
Keyword(s):  
Magnetic Fields ◽  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray

scholarly journals A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC?

2012 ◽  
Vol 537 ◽  
pp. A76 ◽  
Author(s):  
R. Sturm ◽  
F. Haberl ◽  
W. Pietsch ◽  
M. J. Coe ◽  
S. Mereghetti ◽  
...  
Keyword(s):  
White Dwarf ◽  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray

scholarly journals An optical and X-ray study of the counterpart to the Small Magellanic Cloud X-ray binary pulsar system SXP327

2008 ◽  
Vol 387 (2) ◽  
pp. 724-728 ◽  
Author(s):  
M. J. Coe ◽  
M. Schurch ◽  
R. H. D. Corbet ◽  
J. Galache ◽  
V. A. McBride ◽  
...  
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray ◽  
Binary Pulsar

scholarly journals Confirmation of six Be X-ray binaries in the Small Magellanic Cloud

2017 ◽  
Vol 467 (2) ◽  
pp. 1526-1530 ◽  
Author(s):  
V. A. McBride ◽  
A. González-Galán ◽  
A. J. Bird ◽  
M. J. Coe ◽  
E. S. Bartlett ◽  
...  
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray ◽  
X Ray Binaries

scholarly journals The Small Magellanic Cloud, Supersoft X‐Ray Binary 1E 0035.4−7230 (SMC 13)

1997 ◽  
Vol 489 (2) ◽  
pp. 903-911 ◽  
Author(s):  
David Crampton ◽  
J. B. Hutchings ◽  
A. P. Cowley ◽  
P. C. Schmidtke
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray

Deep X-ray survey of the Small Magellanic Cloud

1979 ◽  
Vol 227 ◽  
pp. 54 ◽  
Author(s):  
G. Clark ◽  
F. Li ◽  
J. van Paradijs
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray

Deep Einstein X-ray imagery of the Small Magellanic Cloud

1987 ◽  
Vol 317 ◽  
pp. 152 ◽  
Author(s):  
Frederick C. Bruhweiler ◽  
Daniel A., III Klinglesmith ◽  
Theodore R. Gull ◽  
Sabatino Sofia
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
X Ray

scholarly journals On the geometry of the X-ray emission from pulsars: the changing aspect of the Be/X-ray pulsar SXP348

2019 ◽  
Vol 486 (3) ◽  
pp. 3248-3258
Author(s):  
R Cappallo ◽  
S G T Laycock ◽  
D M Christodoulou ◽  
M J Coe ◽  
A Zezas
Keyword(s):  
Binary System ◽  
Point Source ◽  
Geometric Model ◽  
Magellanic Cloud ◽  
High Mass ◽  
Small Magellanic Cloud ◽  
X Ray ◽  
Spin Period ◽  
The Past ◽  
Model Fits

ABSTRACT The X-ray source SXP348 is a high-mass X-ray binary system in the Small Magellanic Cloud. Since its 1998 discovery by BeppoSAX, this pulsar has exhibited a spin period of ∼340−350 s. In an effort to determine the orientation and magnetic geometry of this source, we used our geometric model Polestar to fit 71 separate pulse profiles extracted from archival Chandra and XMM-Newton observations over the past two decades. During 2002, pulsations ceased being detectable for nine months despite the source remaining in a bright state. When pulsations resumed, our model fits changed, displaying a change in accretion geometry. Furthermore, in 2006, detectable pulsations again ceased, with 2011 marking the last positive detection of SXP348 as a point source. These profile fits will be released for public use as part of the database of Magellanic Cloud pulsars.

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