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    51. http://star.arm.ac.uk/administration/business-plan/2009-2010/bp2009.pdf
    ... investigations of the dynamical evolution of new classes of TNO in the Edgeworth-Kuiper belt and inner Oort cloud, also extending our understanding of the Oort cloud to include spiral-arm and molecular cloud perturbations over the age of the solar system ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/administration/business-plan/2009-2010/bp2009.pdf -- 353.2 Кб -- 20.04.2009
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    52. IAJ: Product Reviews
    ... Topics include accretion disks, molecular clouds, atomic and ionised media, the galactic halo, elliptical and spiral galaxies. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/iaj/reviews/rev26n2.html -- 39.7 Кб -- 06.07.1999
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    53. http://star.arm.ac.uk/preprints/2008/519.pdf
    ... The favoured hypothesis is the fossil field model, which proposes that the magnetic fields are relics of fields present in the molecular clouds from which these stars formed. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2008/519.pdf -- 205.4 Кб -- 29.02.2008
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    54. http://star.arm.ac.uk/annrep/annrep2003/annrep2003.pdf
    ... During passages of the solar system through cold molecular clouds, these life-bearing meteoroids may be incorporated into new ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/annrep/annrep2003/annrep2003.pdf -- 1755.5 Кб -- 18.05.2004
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    55. http://star.arm.ac.uk/~meb/riskpap/riskpap03.doc
    ... Their orbits are more uncertain in the long term owing to perturbations by occasional 'random' close approaches of distant stars and molecular clouds to our solar system, and by the systematic gravitational perturbations of the Galaxy as a whole. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~meb/riskpap/riskpap03.doc -- 103.5 Кб -- 22.10.2010
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    56. http://star.arm.ac.uk/nibulletin/2014/Apr01.html
    ... ТљТљ Abstract: Young starsТљform as the result of the collapse of a high density "core" within a molecular cloud. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2014/Apr01.html -- 31.7 Кб -- 01.04.2014
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    57. http://star.arm.ac.uk/preprints/2014/655.pdf
    ... Furthermore, the width of the filters and the errors of the observed fluxes are given. molecular cloud. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2014/655.pdf -- 720.9 Кб -- 18.09.2014
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    58. http://star.arm.ac.uk/preprints/2010/558.pdf
    ... It is more likely that these differences are real and are related to how the molecular cloud collapsed: low density cores suggest formation by triggering or the interaction of gas motions, while gravitational collapse typically results in higher densities ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2010/558.pdf -- 939.7 Кб -- 16.03.2010
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    59. http://star.arm.ac.uk/preprints/386c.ps
    ... Introduction In the earliest stages of star formation -- the soнcalled Class 0 and Class 1 phases -- protostars are still deeply embedded in their parental molecular cloud cores. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/386c.ps -- 696.7 Кб -- 17.09.2003
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    60. http://star.arm.ac.uk/preprints/2013/639.pdf
    ... 16. The 1.3 mm flux is taken as upper limit as it might be dominated by cold dust emission of the molecular cloud behind the nebula. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2013/639.pdf -- 794.6 Кб -- 09.09.2013
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