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    31. http://www.arcetri.astro.it/science/solar/papers/falchi.helium.pdf
    ... The values quoted ab ove refer to the outer convection zone and to the photosphere. ... in b oth lines is originated in the photosphere, which in the quiet Sun results in a ... In particular, the resulting photosphere could not b e constrained by our ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/solar/papers/falchi.helium.pdf -- 244.5 Кб -- 29.11.2004
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    32. http://www.arcetri.astro.it/science/solar/papers/landolfi.ApJ.573.pdf
    ... the incident radiation field coming from the underlying photosphere and illuminating the scattering atoms be spectrally flat ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/solar/papers/landolfi.ApJ.573.pdf -- 238.9 Кб -- 16.01.2003
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    33. http://www.arcetri.astro.it/~lt/preprints/g3520/g35.ps.gz
    ... this is the most difficult part of the spec­ trum, since the photosphere of an early type star, the ion­ ized gas and the dust ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g3520/g35.ps.gz -- 330.2 Кб -- 11.09.2007
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    34. Report about the Solar Eclipse on August 11, 1999
    ... The last two frames show the low chromosphere and then the photosphere emerging at 3rd contact. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/report-hq.html -- 30.3 Кб -- 29.12.2000
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    35. http://www.arcetri.astro.it/~lt/projects/kona.ps.gz
    ... In some young BDs, emission in excess of that due to the photosphere has been detected in the near (Muench et al. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/kona.ps.gz -- 37.4 Кб -- 11.09.2007
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    36. http://www.arcetri.astro.it/~lt/preprints/p45maser/p45maser.ps.gz
    ... The NIR observations are expected to trace not the stellar photosphere, which would be too extincted to be detectable, but the hottest layers of the dust cocoon in which the newborn star is embedded (Felli & Testi 1996). ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/p45maser/p45maser.ps.gz -- 74.0 Кб -- 11.09.2007
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    37. http://www.arcetri.astro.it/~sperello/AA518_L50.pdf
    ... The fitted model components are the stellar photosphere, and dusty circumstellar envelope (CE). The spectrum of NGC 4371 is shifted by 0.2 dex. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA518_L50.pdf -- 133.2 Кб -- 19.07.2010
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    38. http://www.arcetri.astro.it/~palla/webpage/GES_accretion2015.pdf
    ... high and the star has a sufficiently thin convective envelope, such events may result in a modification of the chemical composition of the stellar photosphere in an observable way, enhancing it with elements that were abundant in the accreted mass ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~palla/webpage/GES_accretion2015.pdf -- 170.8 Кб -- 04.11.2015
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    39. http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf
    ... by VLTI/AMBER spectrointerferometry Astronomy & Astrophysics 488, L67 (2008) · Massi F., Codella C., Brand J., Di Fabrizio L., Wouterloot J. G. A. "NIR spectroscopy of the low-mass YSO CB230­A and its jet: cold photosphere or an active accretion disk ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf -- 112.1 Кб -- 02.12.2015
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    40. http://www.arcetri.astro.it/science/solar/papers/falchi.AA.387.pdf
    ... Time dep endence of the atmospheric parameters During the flare the atmosphere changes only above 600 km (measured from the point where 5000 = 1), while the layers from the photosphere to the low chromosphere remain unchanged. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/solar/papers/falchi.AA.387.pdf -- 275.4 Кб -- 16.01.2003
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