354 citations · 1.4k across the 33 of their papers we have counts for
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SXP 1062, a young Be X-ray binary pulsar with long spin period; Implications for the neutron star birth spin
F. Haberl, R. Sturm, M. D. Filipovic +2
(shortened) The SMC is ideally suited to investigating the recent star formation history from X-ray source population studies. It harbours a large number of Be/X-ray binaries, and…
A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC?
R. Sturm, F. Haberl, W. Pietsch +5
The Small Magellanic Cloud (SMC) hosts a large number of Be/X-ray binaries, however no Be/white dwarf system is known so far, although population synthesis calculations predict tha…
Evolution and Hydrodynamics of the Very-Broad X-ray Line Emission in SN 1987A
D. Dewey, V. V. Dwarkadas, F. Haberl +2
Observations of SN 1987A by the Chandra High Energy Transmission Grating (HETG) in 1999 and the XMM-Newton Reflection Grating Spectrometer (RGS) in 2003 show very broad (v-b) lines…
Highly absorbed X-ray binaries in the Small Magellanic Cloud
G. Novara, N. La Palombara, S. Mereghetti +12
Many of the high mass X-ray binaries (HMXRBs) discovered in recent years in our Galaxy are characterized by a high absorption, most likely intrinsic to the system, which hampers th…
IKT 16: A Composite SNR in the SMC
R. A. Owen, M. D. Filipovic, J. Ballet +11
Aims: IKT 16 is an X-ray and radio-faint supernova remnant (SNR) in the Small Magellanic Cloud (SMC). A previous X-ray study of this SNR found a hard X-ray source near its centre.…
The XMM-Newton survey of the Small Magellanic Cloud: XMMUJ005011.2-730026 = SXP214, a Be/X-ray binary pulsar
M. J. Coe, F. Haberl, R. Sturm +10
In the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), a region to the east of the emission nebula N19 was observed in November 2009. To search for new candida…