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    121. http://star.arm.ac.uk/~csj/papers/conference/2002_WD13_merger.ps
    ... ends, and the helium shell has su uciently reduced the helium envelope mass, the star contracts to become a white dwarf ... The majority of EHes and RCrB stars are single low-mass supergiants with temperatures between 7 000 and 35 000 K, luminosities ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/conference/2002_WD13_merger.ps -- 84.7 Кб -- 06.08.2002
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    122. http://star.arm.ac.uk/~csj/papers/journal/H3269.PS
    ... cool companions identify them as main-sequence stars with masses in the range 0.8{ 1 ... of the binary systems are sdB stars with typical masses of  0:5M (Heber et al ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/journal/H3269.PS -- 605.0 Кб -- 18.01.2002
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    123. annrep2004
    ... Stealth Comets . M.D. Smith . High-Mass Star Formation . Low-Mass Star Formation . Jets . Stellar Outflows and Shocks . ... Stealth Comets . M.D. Smith . High-Mass Star Formation . Low-Mass Star Formation . Jets . Stellar Outflows and Shocks . ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2004/annrep2004.html -- 12.3 Кб -- 11.05.2006
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    124. http://star.arm.ac.uk/preprints/2009/538.pdf
    ... b e able to measure the mass of the neutron stars in AMSPs, and confirm their exp ... to measure the radial velocity of the low mass secondary star (M2 0.05 M ; Bildsten ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2009/538.pdf -- 802.8 Кб -- 27.01.2009
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    125. http://star.arm.ac.uk/jobs/2011/EUNAWE/npm_obs_general_info.pdf
    ... the chromosphere and corona, and Sun-Earth relationships including climate; 4 · Stellar Astrophysics: including hot stars, massive stars, stellar winds, degenerate and helium stars, asteroseismology, studies of binary stars (including their origins ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/jobs/2011/EUNAWE/npm_obs_general_info.pdf -- 70.4 Кб -- 05.07.2011
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    126. http://star.arm.ac.uk/~csj/nuffield/reports/2012_McCarney.pdf
    ... light curves produced by the stars (whose masses should also be determined), and ... hypothesise a cool companion Star B as an M-dwarf, whose mass can also be estimated ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/nuffield/reports/2012_McCarney.pdf -- 1375.4 Кб -- 11.09.2012
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    127. http://star.arm.ac.uk/preprints/307c.ps
    ... such as the mass-luminosity relation for main- sequence stars or a core-mass shell-luminosity relation for shell-burning stars ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/307c.ps -- 318.2 Кб -- 07.03.2006
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    128. Armagh Observatory
    ... Eight stages to the formation of a low mass star like our sun. The Stages:. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/sketch.html -- 4.8 Кб -- 04.11.2009
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    129. http://star.arm.ac.uk/preprints/488.pdf
    ... Subject headings: radio continuum: stars ­ stars: low-mass, brown dwarfs ­ stars: activity ­ stars: magnetic fields ­ stars ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/488.pdf -- 307.2 Кб -- 22.08.2006
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    130. Gamma- ray bursts
    ... Stan Woosley believes that bursts happen when a very massive star suddenly turns into a black hole. ... edge of the universe, are formed by either a very massive star collapsing or two neutron stars colliding, and the most likely ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/essays/grb.html -- 15.4 Кб -- 01.10.2012
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