... Magnetic braking of the 1 Ori C main component Y.Balega, V.Leushin, and G.Weigelt Special Astrophysical Observatory, Nizhnij Arkhyz Max-Planck-Institute for Radioastronomy, Bonn 2010 1 Ori C the youngest and the nearest high-mass star P = 11.26 yrs T ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf -- 453.0 Кб -- 26.01.2011 Похожие документы
... Sco OB Ori b = -9 0 ° PSRs+ Geminga+ M7 PSRs- Clearly several rich OB associations start to dominate in the spatial distribution 16 INSs and local surrounding Massive star population in the Solar vicinity (up to 2 kpc) is dominated by OB associations. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/09-popov.pdf -- 2545.7 Кб -- 30.01.2008 Похожие документы