... N5430 M.H.Finger et al (1992) [25] K.Tamura et al ApJ 389,676 (1992) [26] T.Aoki et al PASJ 44,641 (1992) [27] V.M.Loznikov et al., Pisma Astr. ...
... N5430 M.H.Finger et al (1992) [25] K.Tamura et al ApJ 389,676 (1992) [26] T.Aoki et al PASJ 44,641 (1992) [27] V.M.Loznikov et al., Pisma Astr. ...
... 2003), 2.4±0.27M # for 4U 1700 37 (Clark et al. 2002; see also Heineke et al. 2003; van Kerkwijk 2004). ... as they are ex 1 This range is based on the two estimates given in (Quaintrell et al. 2003): 1.88 ± 0.13 and 2.27 ± 0.17 M ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/ouyed/skyrm_aa6.ps -- 1034.9 Кб -- 14.12.2004 Похожие документы
... 2003), 2.4±0.27M # for 4U 170037 (Clark et al. 2002; see also Heineke et al. 2003, van Kerkwijk 2004). ... 3.45 M # and R = 1 This range is based on the two estimates given in Quaintrell et al. (2003): 1.88 ± 0.13 and 2.27 ± 0.17 M ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/ouyed/skyrm_aa5.ps -- 1052.9 Кб -- 11.12.2004 Похожие документы
... around 7-10 M , but the potentially cover a relatively wide range from 3 up to 50 solar masses [2], [27] (see the theoretical ... 27] M.E. Prokhorov, K.A. Postnov, Why NS and BH mass distribution is bimodal?, to appear in Odessa Astr. ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/icga/icga.ps -- 141.2 Кб -- 19.12.2001 Похожие документы
... 64 3.22 0.68 L MassShed 0.116 0.443 1.80 1.25 2.70 3.27 0.76 M MassShed 0.091 0.367 1.74 1.49 1.80 2.10 0.81 The second and the ... Ruderman, M., Zhu, T. & Chen, K. 1998, ApJ, 492, 267 Spin and magnetism in old neutron stars 27 69. ...
... Style 27 Sako, M., Kahn, S. M., Paerels, F., & Liedahl, D. A. 2000, ApJ, 543, L115 Sambruna, R. M., Brandt, W. N., Chartas, G., Netzer, H., Kaspi, S., Garmire, G. P., Nousek, J. A., & Weaver, K. A. 2001, ApJ, 546, L9 Sarazin, C. L., Irwin, J. A ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/images/chandra/chandra2001/paper.ps -- 185.5 Кб -- 15.10.2001 Похожие документы