activity
20092017
most citedStar formation history and X-ray binary populations: the case of the Small Magellanic Cloud

110 citations · 392 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2017★ 5 cited

Hα imaging for BeXRBs in the Small Magellanic Cloud

Grigoris Maravelias, Andreas Zezas, Vallia Antoniou +2

The Small Magellanic Cloud (SMC) hosts a large number of high-mass X-ray binaries, and in particular of Be/X-ray Binaries (BeXRBs; neutron stars orbiting OBe-type stars), offering…

astro-ph.HE2013★ 23 cited

Optical spectra of 5 new Be/X-ray Binaries in the Small Magellanic Cloud and the link of the supergiant B[e] star LHA 115-S 18 with an X-ray source

Grigoris Maravelias, Andreas Zezas, Vallia Antoniou +1

The Small Magellanic Cloud (SMC) is well known to harbor a large number of High-Mass X-ray Binaries (HMXBs). The identification of their optical counterparts provides information o…

astro-ph.HE2013★ 95 cited

The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue

R. Sturm, F. Haberl, W. Pietsch +8

Local-Group galaxies provide access to samples of X-ray source populations of whole galaxies. The XMM-Newton survey of the Small Magellanic Cloud (SMC) completely covers the bar an…

astro-ph.HE2012★ 23 cited

Supersoft X-rays reveal a classical nova in the M 31 globular cluster Bol 126

M. Henze, W. Pietsch, F. Haberl +17

[Abridged] Classical novae (CNe) represent the main class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M 31. Only three confirmed novae and th…

astro-ph.HE2010★ 18 cited

The XMM-Newton survey of the Small Magellanic Cloud: Discovery of the 11.866 s Be/X-ray binary pulsar XMMUJ004814.0-732204 (SXP11.87)

R. Sturm, F. Haberl, M. J. Coe +12

One of the goals of the XMM-Newton survey of the Small Magellanic Cloud is the study of the Be/X-ray binary population. During one of our first survey observations a bright new tra…

astro-ph.HE2010★ 61 cited

X-ray monitoring of classical novae in the central region of M 31. II. Autumn and winter 2007/2008 and 2008/2009

M. Henze, W. Pietsch, F. Haberl +7

[Abridged] Classical novae (CNe) represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M 31. We performed a dedicated monitor…

astro-ph.HE2010★ 110 cited

Star formation history and X-ray binary populations: the case of the Small Magellanic Cloud

Vallia Antoniou, Andreas Zezas, Despina Hatzidimitriou +1

Using Chandra, XMM-Newton, and optical photometric catalogs we study the young X-ray binary (XRB) populations of the Small Magellanic Cloud. We find that the Be/X-ray binaries (Be-…

astro-ph.HE2009★ 47 cited

Optical spectroscopy of 20 Be/X-ray Binaries in the Small Magellanic Cloud

Vallia Antoniou, Despina Hatzidimitriou, Andreas Zezas +1

We present a large sample (20 in total) of optical spectra of Small Magellanic Cloud (SMC) High-Mass X-ray Binaries obtained with the 2dF spectrograph at the Anglo-Australian Teles…

astro-ph.HE2009★ 3 cited

Recent discoveries of supersoft X-ray sources in M 31

M. Henze, W. Pietsch, F. Haberl +9

Classical novae (CNe) have recently been reported to represent the major class of supersoft X-ray sources (SSSs) in the central area of our neighbouring galaxy M 31. This paper pre…

astro-ph.HE2009★ 7 cited

Spectroscopy of the bright optical counterparts of X-ray sources in the direction of M 31. II

Paolo Bonfini, Despina Hatzidimitriou, Wolfgang Pietsch +1

A recent survey of the Local Group spiral galaxy M 31 with XMM-Newton yielded a large number of X-ray sources. This is the second in a series of papers with the aim of identifying…