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Constraining the geometry of the neutron star RX J1856.5−3754

✍ Scribed by Wynn C. G. Ho


Book ID
110842124
Publisher
John Wiley and Sons
Year
2007
Tongue
English
Weight
188 KB
Volume
380
Category
Article
ISSN
0035-8711

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On the recently discovered pulsations fr
✍ N. Chkheidze; D. Lomiashvili 📂 Article 📅 2008 🏛 Elsevier Science 🌐 English ⚖ 147 KB

An explanation of the recently discovered 7 s pulsations from the isolated neutron star RX J1856.5-3754 is presented. It is assumed that the real spin period of this source is %1 s, whereas the observed spin-modulation is caused by the presence of a nearly transverse, very low frequency drift waves