... in the immediate vicinity of stellar objects: where a high enough ionizing flux is present, generally in later type TTauri stars, photoionization can support an embedded H II region (Churchwell 1990); a fully ionized stellar wind, again associated more ...
... nuclear burning, and with masses similar to the Sun, are known as TTauri stars ... with these more luminous young stars, TTauri stars undergoing bursts of enhanced ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf -- 1989.2 Кб -- 25.06.2007 Похожие документы
... A. Quirrenbach, D. F. Buscher, D. Mozurkewich, C. A. Hummel, and J. T. Armstrong, Maximum-entropy maps of the be shell star н¶ tauri from optical long-baseline interferometry, Astron. ...
... Herbig Ae/Be, LBV & TT Tauri 162 62 sup ergiants 5073 1253 Egret stars with d<10 mas 143 8 Fracassini et al. ... van den Ancker, M. E., Maira, A., Thґ, P. S., Djie, H. R. E. T. A., Redondo, I., Eiroa, C., & e Molster, F. J. 2001, A&A, 380 ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-50-c.pdf -- 1649.1 Кб -- 20.02.2013 Похожие документы