✦ LIBER ✦

Observation of X-ray eclipses from LMC X-4

✍ Scribed by LI, F.; RAPPAPORT, S.; EPSTEIN, A.

Book ID: 109708145
Publisher: Nature Publishing Group
Year: 1978
Tongue: English
Weight: 242 KB
Volume: 271
Category: Article
ISSN: 0028-0836
DOI: 10.1038/271037a0

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Discovery of eclipsing nature of LMC X-4

✍ WHITE, N.E. 📂 Article 📅 1978 🏛 Nature Publishing Group 🌐 English ⚖ 320 KB

First observation of ultra-high-energy γ

First observation of ultra-high-energy γ rays from LMC X-4

✍ Protheroe, R. J.; Clay, R. W. 📂 Article 📅 1985 🏛 Nature Publishing Group 🌐 English ⚖ 361 KB

Simulataneous X-ray and optical observat

Simulataneous X-ray and optical observations of LMC X-2

✍ J.M. Bonnet-Bidaud; C. Motch; K. Beuermann; M. Pakull; A. Parmar; M. van der Kli 📂 Article 📅 1988 🏛 Elsevier Science 🌐 English ⚖ 339 KB

Long-term INTEGRAL and RXTE observations

Long-term INTEGRAL and RXTE observations of the X-ray pulsar LMC X-4

✍ S. S. Tsygankov; A. A. Lutovinov 📂 Article 📅 2005 🏛 Springer 🌐 English ⚖ 323 KB

LMC X-4, AO538-66 and surrounding X-ray

LMC X-4, AO538-66 and surrounding X-ray sources observed with EXOSAT

✍ M. Pakull; H. Brunner; W. Pietsch; A. Staubert; K. Beuermann; M. Klis; J. M. Bon 📂 Article 📅 1985 🏛 Springer Netherlands 🌐 English ⚖ 194 KB

Repeated observations of LMC X-4 with EXOSAT were carried out in 1983/84 in order to study its 30.5 day cycle and to cover the expected outbursts of the recurrent LMC transient A0538-66. The latter source was inactive during our campaign although a variable circumstellar envelope was still present a

LMC X-4: 13.5 s pulsations and an X-ray

LMC X-4: 13.5 s pulsations and an X-ray flare observed by EXOSAT

✍ W. Pietsch; M. Pakull; W. Voges; R. Staubert 📂 Article 📅 1985 🏛 Springer Netherlands 🌐 English ⚖ 340 KB

EXOSAT observed LMC X-4 on November 17/19, 1983 for one 1.4 day binary period during the high state of the 30.5 day cycle. An eclipse with sharp ingress and slow egress was detected with an eclipse angle of 27.1+1.0 dgr. In the medium energy experiment the source showed 'a hard power law spectrum. O