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    71. Report about the Solar Eclipse on August 11, 1999 | ESO Ireland
    ... The last two frames show the low chromosphere and then the photosphere emerging at 3rd contact. ...
    [ Сохраненная копия ]  Ссылки http://www.eso.org/public/ireland/news/eso9941/ -- 97.4 Кб -- 11.04.2016
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    72. Report about the Solar Eclipse on August 11, 1999 | ESO United Kingdom
    ... The last two frames show the low chromosphere and then the photosphere emerging at 3rd contact. ...
    [ Сохраненная копия ]  Ссылки http://www.eso.org/public/unitedkingdom/news/eso9941/ -- 97.5 Кб -- 13.04.2016
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    73. Report about the Solar Eclipse on August 11, 1999 | ESO United States
    ... The last two frames show the low chromosphere and then the photosphere emerging at 3rd contact. ...
    [ Сохраненная копия ]  Ссылки http://www.eso.org/public/usa/news/eso9941/ -- 97.4 Кб -- 11.04.2016
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    74. http://www.eso.org/~rsiebenm/FTP/RSiebenmorgenDust.pdf
    ... elements in the ISM are similar to those measured in the photosphere of the Sun ... the elemental abundances in the solar photosphere (Asplund et al. 2009) and that of ...
    [ Текст ]  Ссылки http://www.eso.org/~rsiebenm/FTP/RSiebenmorgenDust.pdf -- 795.6 Кб -- 28.01.2014
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    75. http://www.eso.org/~fcomeron/cham_companions.pdf
    ... if the objects were cool enough for their atmospheres to be dust-depleted owing to the sedimentation of dust grains below the photosphere (Burrows 2009), which has been proposed to mark the transition between the L and T spectral types (Kirkpatrick 2005 ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/cham_companions.pdf -- 1012.7 Кб -- 29.11.2011
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    76. http://www.eso.org/~bleibund/papers/VLTIII.ps
    ... 1999). The spectrum is not formed in a regular photosphere, but is the result of complicated scattering of photons out of the ejecta. ...
    [ Текст ]  Ссылки http://www.eso.org/~bleibund/papers/VLTIII.ps -- 202.9 Кб -- 07.01.2001
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    77. http://www.eso.org/~fpatat/science/sn06X/924.pdf
    ... in the case of SN 2006X, transverse motions in the absorbing material and line-of-sight effects due to the fast SN photosphere expansion (typically 104 km s-1) can be definitely excluded, because they would cause variations in all absorption features ...
    [ Текст ]  Ссылки http://www.eso.org/~fpatat/science/sn06X/924.pdf -- 199.7 Кб -- 22.08.2007
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    78. http://www.eso.org/~bleibund/papers/GRandG.ps
    ... by Baade (1926), originally done for Cepheid stars, the expanding photosphere method (EPM; Kirshner & Kwan 1974, Schmidt et al ...
    [ Текст ]  Ссылки http://www.eso.org/~bleibund/papers/GRandG.ps -- 759.4 Кб -- 28.11.2007
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    79. http://www.eso.org/~bleibund/papers/Freiburg.ps
    ... Following early work by Baade (1926), originally done for Cepheid stars, the expanding photosphere method (EPM; East­ man et al. 1996) has been applied to several supernovae. ...
    [ Текст ]  Ссылки http://www.eso.org/~bleibund/papers/Freiburg.ps -- 946.7 Кб -- 05.07.2004
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    80. http://www.eso.org/~fcomeron/cham.ps
    ... NC98, which is dominated by a broad depression between the H and K bands due to water absorption in the photosphere of the star ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/cham.ps -- 2327.9 Кб -- 19.02.1999
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