1E 1207.4–5209-LIKE RADIO-QUIET NEUTRON STARS

DOI10.1142/S0218271809015783zbMath1180.85005MaRDI QIDQ3405928

Aşkin Ankay, Arzu Mert Ankay, Enise Nihal Ercan, Murat Hudaverdi

Publication date: 12 February 2010

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

zbMATH Keywords

pulsarneutron star

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Temporal evolution of isolated pulsars; Age-Tau problem

Cites Work

• THE STRONG MAGNETIC FIELD DECAY AND EVOLUTION OF RADIO PULSARS ON THE P–Ṗ DIAGRAM
• POSSIBLE EVOLUTION OF DIM RADIO-QUIET NEUTRON STAR 1E 1207.4-5209 BASED ON A B-DECAY MODEL
• 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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