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Home All issues A&A, 406 2 (2003) 471-481 Article references

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Cited article:

RX J0529.8−6556: a BeXRB pulsar with an evolving optical period and out of phase X-ray outbursts

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Monthly Notices of the Royal Astronomical Society 503 (4) 6187 (2021)
https://doi.org/10.1093/mnras/stab807

Identification of high-mass X-ray binaries selected from XMM–Newton observations of the LMC

N van Jaarsveld, D A H Buckley, V A McBride, et al.
Monthly Notices of the Royal Astronomical Society 475 (3) 3253 (2018)
https://doi.org/10.1093/mnras/stx3270

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

V. Antoniou and A. Zezas
Monthly Notices of the Royal Astronomical Society 459 (1) 528 (2016)
https://doi.org/10.1093/mnras/stw167

Constraining compactness and magnetic field geometry of X-ray pulsars from the statistics of their pulse profiles

M. Annala and J. Poutanen
Astronomy and Astrophysics 520 A76 (2010)
https://doi.org/10.1051/0004-6361/200912773

AKARI IRC Survey of the Large Magellanic Cloud: Outline of the Survey and Initial Results

Yoshifusa Ita, Takashi Onaka, Daisuke Kato, Toshihiko TanabÉ, Itsuki Sakon, Hidehiro Kaneda, Akiko Kawamura, Takashi Shimonishi, Takehiko Wada, Fumihiko Usui, Bon-Chul Koo, Mikako Matsuura, Hidenori Takahashi, Yoshikazu Nakada, Tetsuo Hasegawa and Motohide Tamura
Publications of the Astronomical Society of Japan 60 (sp2) S435 (2008)
https://doi.org/10.1093/pasj/60.sp2.S435

An INTEGRAL hard X-ray survey of the Large Magellanic Cloud

D. Götz, S. Mereghetti, D. Merlini, L. Sidoli and T. Belloni
Astronomy & Astrophysics 448 (3) 873 (2006)
https://doi.org/10.1051/0004-6361:20053744

An XMM-Newton survey of the Local Group galaxy M 33 – variability of the detected sources

Z. Misanovic, W. Pietsch, F. Haberl, et al.
Astronomy & Astrophysics 448 (3) 1247 (2006)
https://doi.org/10.1051/0004-6361:20053745

XMM-Newton observation of the Be/neutron star system RX J0146.9+6121: a soft X-ray excess in a low luminosity accreting pulsar

N. La Palombara and S. Mereghetti
Astronomy & Astrophysics 455 (1) 283 (2006)
https://doi.org/10.1051/0004-6361:20065107

High mass X-ray binaries in the LMC: Dependence on the stellar population age and the “propeller” effect

P. Shtykovskiy and M. Gilfanov
Astronomy & Astrophysics 431 (2) 597 (2005)
https://doi.org/10.1051/0004-6361:20041074

XMM‐NewtonObservations of the M31 Northern Disk: Properties of Selected X‐Ray Sources and Unresolved Emission

Sergey Trudolyubov, Oleg Kotov, William Priedhorsky, France Cordova and Keith Mason
The Astrophysical Journal 634 (1) 314 (2005)
https://doi.org/10.1086/496940

Discovery of 1323 s pulsations from RX J0103.6–7201: The longest period X-ray pulsar in the SMC

F. Haberl and W. Pietsch
Astronomy & Astrophysics 438 (1) 211 (2005)
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Discovery of a Peculiar Pulsar in the Small Magellanic Cloud

Masaru Ueno, Hiroya Yamaguchi, Shin-ichiro Takagi, Jun Yokogawa and Katsuji Koyama
Publications of the Astronomical Society of Japan 56 (1) 175 (2004)
https://doi.org/10.1093/pasj/56.1.175

Origin of the Soft Excess in X‐Ray Pulsars

Ryan C. Hickox, Ramesh Narayan and Timothy R. Kallman
The Astrophysical Journal 614 (2) 881 (2004)
https://doi.org/10.1086/423928

Two long-period X-ray pulsars detected in the SMC field around

F. Haberl, W. Pietsch, N. Schartel, P. Rodriguez and R. H. D. Corbet
Astronomy & Astrophysics 420 (3) L19 (2004)
https://doi.org/10.1051/0004-6361:20040156

Timing and spectral changes of the Be X-ray transient EXO 0531-6609.2 through high and low state

N. Rea, G. L. Israel, T. Di Salvo, L. Burderi and G. Cocozza
Astronomy & Astrophysics 421 (1) 235 (2004)
https://doi.org/10.1051/0004-6361:20035685

Timing and Spectral Studies of the Transient X‐Ray Pulsar EXO 053109−6609.2 withASCAandBeppoSAX

B. Paul, S. N. A. Jaaffery, S. Naik and P. C. Agrawal
The Astrophysical Journal 602 (2) 913 (2004)
https://doi.org/10.1086/381161

Nuclear Activity and Massive Star Formation in the Low‐Luminosity Active Galactic Nucleus NGC 4303:ChandraX‐Ray Observations

E. Jimenez‐Bailon, M. Santos‐Lleo, J. M. Mas‐Hesse, et al.
The Astrophysical Journal 593 (1) 127 (2003)
https://doi.org/10.1086/376554