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    • 1 | 2 | След.

    1. http://www.mrao.cam.ac.uk/~anthony/latex/Mazzali.ps
    ... For smaller epochs the temperature of the ejecta is too high, or the photosphere must be at velocities so large that there is not enough material above it to form strong absorption lines. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Mazzali.ps -- 26.2 Кб -- 24.06.2000
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    2. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HCegla.pdf
    ... These components are constructed by averaging Fe i 6302 е magnetically sensitive absorption line profiles output from detailed radiative transport calculations of the solar photosphere. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HCegla.pdf -- 2916.7 Кб -- 16.04.2014
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    3. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/mnr3438.pdf
    ... circumstellar gas they detect is transported from the photosphere of the star, and so one possibility would be that these, together with localized heating, lead to less opaque channels through which the emission from the photosphere can escape ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/mnr3438.pdf -- 449.7 Кб -- 20.02.2013
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    4. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-95-letter.ps
    ... correspond to areas of elevated temperature in the stellar photosphere, whose apparent contrast with the surrounding disc is ... photospheric layers, it is clear that any area of enhanced temperature in the deeper photosphere can be completely masked ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-95-letter.ps -- 933.4 Кб -- 20.02.2013
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    5. Chris Haniff's Astronomy Page
    ... Optical Aperture Synthetic Imaging of The Photosphere Molecular Atmosphere of Mira'', Haniff, C.A., Ghez, A.M., Gorham, P.W., Kulkarni, S.R., Matthews, K., Neugebauer, G. 1992 Astron. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~cah/astronomy.html -- 25.0 Кб -- 08.11.2002
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    6. John Young's PhD Thesis
    ... Optical aperture synthetic images of the photosphere and molecular atmosphere of Mira . Astron. J. , 103 , 1662-1667, 1992. C . ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/thesis.html -- 49.8 Кб -- 08.02.2004
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    7. http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf
    ... from which photons can escape (the photosphere) is a substantial fraction of the ... Observations at different wavelengths probe different layers within the photosphere. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf -- 2354.4 Кб -- 20.07.1999
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    8. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/4006-55.pdf
    ... Smaller areas for the hotspots imply that their temperatures must be greater than T1290 , and so the bright features do trace pockets of hot gas within the deeper photosphere. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/4006-55.pdf -- 432.4 Кб -- 20.02.2013
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    9. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf
    ... emission.8 By combining short and long baselines simultaneously, VSI will allow a simultaneous measurement of the stellar photosphere and of the circumstellar emission, thereby greatly reducing the time needed to fully characterize the star-disk system ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf -- 273.0 Кб -- 20.02.2013
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    10. http://www.mrao.cam.ac.uk/~eic22/Papers/scaife10.pdf
    ... For young embedded protostars the accretion luminosity will dominate over that from the stellar photosphere. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~eic22/Papers/scaife10.pdf -- 1198.0 Кб -- 03.09.2010
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