... of, e.g., the coalescence of two neutron stars or neutron stars and black holes ... case of a coalescence of two neutron stars or a neutron star and a black hole the ...
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Ссылки http://observ.pereplet.ru/images/evgeny/magneto21jun07Eng.doc -- 683.5 Кб -- 21.06.2007 Похожие документы
... of, e.g., the coalescence of two neutron stars or neutron stars and black holes ... case of a coalescence of two neutron stars or a neutron star and a black hole the ...
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Ссылки http://observ.pereplet.ru/images/evgeny/article/2007/MNRAS.pdf -- 895.1 Кб -- 01.11.2007 Похожие документы
... Population synthesis of a merging of neutron stars yields a similar rate of 10 4 yr ... two ways: via a collision of two neutron stars (Lipunova & Lipunov 1998) or via the ...
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Ссылки http://observ.pereplet.ru/images/evgeny/article/2007/ApjLettt.pdf -- 201.3 Кб -- 27.09.2007 Похожие документы
... M81 as a candidate [13] for a soft gamma-ray host galaxy is very probable, but we note that the error box is placed outside the spiral arms region, where the progenitor of a highly magnetized neutron star formed. ...
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Ссылки http://observ.pereplet.ru/images/evgeny/article/2007/transacion.pdf -- 211.7 Кб -- 19.10.2007 Похожие документы
... The error box lies outside any spiral arms, where strongly magnetized neutron stars (magnetars, which are thought to be the sources of SGRs) would be likely to form. ...
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Ссылки http://observ.pereplet.ru/images/evgeny/article/2007/statia_AZh_eng3.pdf -- 697.9 Кб -- 22.10.2007 Похожие документы
... The error box lies outside any spiral arms, where strongly magnetized neutron stars (magnetars, which are thought to be the sources of SGRs) would be likely to form. ...