POSSIBLE EVOLUTION OF DIM RADIO-QUIET NEUTRON STAR 1E 1207.4-5209 BASED ON A B-DECAY MODEL

DOI10.1142/S0218271807009383zbMath1119.85301arXiv0706.0831MaRDI QIDQ5297838

Arzu Mert Ankay, Aşkin Ankay, Enise Nihal Ercan

Publication date: 13 July 2007

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0706.0831

zbMATH Keywords

pulsarevolutionneutron star1E 1207.4-5209

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (2)

Temporal evolution of isolated pulsars; Age-Tau problem ⋮ 1E 1207.4–5209-LIKE RADIO-QUIET NEUTRON STARS

Cites Work

• THE STRONG MAGNETIC FIELD DECAY AND EVOLUTION OF RADIO PULSARS ON THE P–Ṗ DIAGRAM
• BIRTH RATES OF DIFFERENT TYPES OF NEUTRON STARS AND POSSIBLE EVOLUTIONS OF THESE OBJECTS
• DEPENDENCE OF THE X-RAY LUMINOSITY AND PULSAR WIND NEBULA ON DIFFERENT PARAMETERS OF PULSARS AND THE EVOLUTIONARY EFFECTS

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