Neutron star dynamics, braking indices and energy dissipation

---

Atıf İçin Kopyala

Alpar M.

SPACE BASED ASTRONOMY: ISO, AGN, RADIOPULSARS AND THE SUN, cilt.21, ss.159-166, 1998 (SCI-Expanded)

• Yayın Türü: Makale / Tam Makale
• Cilt numarası: 21
• Basım Tarihi: 1998
• Doi Numarası: 10.1016/s0273-1177(97)00800-4
• Dergi Adı: SPACE BASED ASTRONOMY: ISO, AGN, RADIOPULSARS AND THE SUN
• Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
• Sayfa Sayıları: ss.159-166
• Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

Models of pulsar glitches and postglich relaxation are reviewed. Implications for braking indices due to internal torques in the neutron star, and energy dissipation by internal torques are discussed. AU recent observations of pulsars with large (Vela pulsar like) glitches and second derivatives are seen to fit with the same glitch dynamics that the Vela pulsar exhibits. (C)1998 COSPAR. Published by Elsevier Science Ltd.