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    41. http://star.arm.ac.uk/ssab-workshop/landstreet/Cluster-project.pdf
    ... in PMS phase (North) · Slowest rotators are cooler ­ lower mass ­ Ap stars that spend longer in PMS phase (Stepien) · Hubrig et ... To find mass of a cluster star, we use Te, determined from Geneva or uvby photometry · We find luminosity using cluster ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/ssab-workshop/landstreet/Cluster-project.pdf -- 1193.5 Кб -- 26.03.2008
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    42. http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-8-pulsars-and-final-overview.pdf
    ... field of order 100 MG A few pulsars form (perhaps from massive stars with extremely large fields on MS) with >100 TG fields ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/lectures/landstreet/slides/Lecture-8-pulsars-and-final-overview.pdf -- 688.4 Кб -- 05.07.2009
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    43. Armagh Observatory
    ... a radius of 1.5 centered on the massive star system HD 206267 (O6.5V), which is the ... classical T Tauri star candidates and (2) constrain the mass accretion rates with an ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2011/573.html -- 6.5 Кб -- 14.03.2011
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    44. Supernova
    ... The deaths of stars . Low Mass stars . Massive stars . Supernovae on white dwarfs . ... The deaths of stars . Low Mass stars . Massive stars . Supernovae on white dwarfs . ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/essays/supernovae.html -- 19.1 Кб -- 02.10.2012
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    45. http://star.arm.ac.uk/~jsv/Mdot.pro
    ... Mass, vinf ; Mass-loss recipe for massive stars including a metallicity dependence ... Mass-loss predictions for O and B stars as a function of metallicity" ; Jorick S ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~jsv/Mdot.pro -- 5.3 Кб -- 02.04.2007
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    46. Armagh Observatory
    ... star is extremely luminous, perhaps 3 million times that of the Sun, is about 150 ... We were very surprised to find such a massive star on its own, and not in a rich ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/2011/monster_star_pr2.html -- 9.1 Кб -- 25.05.2011
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    47. http://star.arm.ac.uk/preprints/2012/624.pdf
    ... winds, which are expected to be stronger in massive stars, are at the origin of this ... of angular momentum of intermediate-mass stars during the PMS phase have been ... of the spin angular momentum of intermediate mass stars during the PMS phase by ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2012/624.pdf -- 542.2 Кб -- 20.11.2012
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    48. Homepage of Gavin Ramsay
    ... Flares stars like the one described in our study (which has a mass around 1/4 of ... the number, duration, energy) are effected by a stars mass, rotation period and age ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~gar/Flares.html -- 3.8 Кб -- 23.11.2015
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    49. http://star.arm.ac.uk/lectures/landstreet/class-outline.pdf
    ... sequence phenomena (stellar activity in chemistry and inhomogeneity in found in the Sun, cool main sequence stars, and of the accompanying low-mass stars, unusual atmospheric more massive stars) Lecture 5 A review of the basic ideas of radiative transfer ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/lectures/landstreet/class-outline.pdf -- 19.2 Кб -- 09.02.2009
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    50. THE EVOLUTIONARY STATUS OF RCBS
    ... In one model, a low-mass star which has finished its evolution as a red giant ... star is a helium white dwarf (HeWD), and the other a carbon/oxygen white dwarf (COWD ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/research/rcb_review/node12.html -- 6.5 Кб -- 25.01.2002
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