... Key words: Stars:latetype -- Stars:massloss --ISM:general -- Infrared:stars ... found in the spectra of early type stars undergoing mass loss at rates of 10 \Gamma5 ...
... of key objects among southern massivestars, specifically the LBVs/hypergiants HD ... and reduction procedures) of luminous and massivestars is given by van Genderen et ...
... Astrophysics Seminar Friday, 27 July 2007 at 12.00 noon SchrЖdinger Lecture Theatre Current problems in massivestar evolution: mass-loss, mixing, magnetic fields and metallicity Dr. Danny Lennon Isaac Newton Group of Telescopes (ING) Canary Islands, Spain ...
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Ссылки http://star.arm.ac.uk/nibulletin/2007/Danny_Lennon_seminar_poster.pdf -- 126.3 Кб -- 25.07.2007 Похожие документы
... Dominant Source of Radio Emission from Very Low MassStars and Brown Dwarfs . Updated 2008 July 4th . ... Discovery of magnetic fields in the very young, massivestars . W601 (NGC 6611) and OI~201 (NGC 2244) . ...
... of massive main sequence stars, they are low massstars (<1.0 M ) in an advanced ... binary helium white dwarf to become a low-mass helium star (Saio & Jeffery 2000 ... the iron-group bump instability where low-mass extreme-helium stars are lo cated ...
... for the radius ratio R2/R1 , the hot starmass M1 and the cool star gravity log g2 ... R 1 is adopted, an estimate for the hot starmass M 1 and the quality of the log g 2 ...
... chromospheric emission lines Fields in more massivestars do affect spectra of stars ... and angular momentum during star formation, with stellar mass loss, and in close ...
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Ссылки http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-1-intro-to-stellar-magnetism.pdf -- 906.8 Кб -- 09.02.2009 Похожие документы
... an SFR 3.5M yr-1 and a total disc mass (in stars) Md 5.2 в 1010 M at the current ep ... This structure and the thin disc mass (in stars) are consistent with the dynamical ...
... for the radius ratio R2 /R1 , the hot starmass M1 and the cool star gravity log g2 ... R2 /R1 is adopted, an estimate for the hot starmass M1 and the quality of the log g ...