메뉴 건너뛰기




Volumn 53, Issue 4, 1996, Pages 1845-1852

Structure of rotating neutron stars with meson condensates

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0348076612     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.53.1845     Document Type: Article
Times cited : (9)

References (43)
  • 7
    • 85035220098 scopus 로고
    • Kyoto Report No. KUNS 1318, unpublished
    • T. Tatsumi, Kyoto Report No. KUNS 1318, 1995 (unpublished).
    • (1995)
    • Tatsumi, T.1
  • 13
    • 85035239375 scopus 로고
    • Ph.D. thesis, SUNY at Stony Brook
    • V. Thorsson, Ph.D. thesis, SUNY at Stony Brook, 1992;
    • (1992)
    • Thorsson, V.1
  • 39
    • 0011401312 scopus 로고
    • G. E. Brown, Nature 336, 519 (1988).
    • (1988) Nature , vol.336 , pp. 519
    • Brown, G.E.1
  • 41
    • 85035210972 scopus 로고    scopus 로고
    • private communication, Prediction of the iron core mass of 1.2 1.8Msub odot determines the mass cut, typically sim 1.4Msub odot, which separates the neutron star or black hole from the supernova ejecta. The place of the mass cut is based on the amounts of (formula presented) Ni and the neutron rich nuclei produced by the explosive nucleosynthesis
    • M. Hashimoto (private communication). Prediction of the iron core mass of 1.2 1.8Msub odot determines the mass cut, typically sim 1.4Msub odot, which separates the neutron star or black hole from the supernova ejecta. The place of the mass cut is based on the amounts of (formula presented) Ni and the neutron rich nuclei produced by the explosive nucleosynthesis.
    • Hashimoto, M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.