... Will consider magnetic pressure, instead of ceRrifugally driven nt co Protostellar/TTauri Jets Two basic models: Flow || to B Why the dichotomy? ...
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Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/liffman.pdf -- 2807.2 Кб -- 16.06.2010 Похожие документы
... J = 1 0) line emission at 89 GHz (3.4 mm) from two young southern disk targets, TW Hya, the closest known classical TTauri star, and HD 100546, a nearby Herbig Be star whose infrared spectr um shows cr ystalline silicates, indicative of comet-like dust ...
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Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p17-37.pdf -- 1956.0 Кб -- 14.07.2003 Похожие документы
... TAURIS, T. & SENNELS, T. "Formation of the binary pulsars PSR B2303+46 and PSR J1141-6545. Young neutron stars with old white dwarf companions". ...
... of magnetic activity and cycles, stellar flares and cosmic ray production and acceleration, as well as dK/dM and TTauri types · Pulsations and mass loss in cool supergiants · Binaries with compact neutron-star or blackhole components, to provide valuable ...
... Manchester, R. N. 1988, MNRAS, 234, 477 Lyne, A. G., Manchester, R. N., Lorimer, D. R., Bailes, M., D'Amico, N., Tauris, T. M., Johnston, S., Bell, J. F., & Nicastro, L. 1998, MNRAS, 295, 743 Lyutikov, M. & Thompson, C. 2005, ApJ, 634, 1223 Manchester, B ...
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Ссылки http://www.atnf.csiro.au/research/conferences/Parkes50th/ProcPapers/manchester.pdf -- 927.1 Кб -- 02.10.2012 Похожие документы