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    81. http://www.eso.org/~bleibund/CV/pap.pdf
    ... A84 Gall, E.E.E., Kotak, R., Leibundgut, B., Taubenberger, S., Hillebrandt, W., Kromer, M.: Applying the expanding photosphere and standardized candle methods to Type II-Plateau supernovae at cosmologically significant redshifts: the distance to SN 2013eq ...
    [ Текст ]  Ссылки http://www.eso.org/~bleibund/CV/pap.pdf -- 213.5 Кб -- 31.03.2016
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    82. http://www.eso.org/~fcomeron/m17_hh.pdf
    ... An alternative possibility to consider is that the observed X-ray emission may not be caused by coronal activity in the photosphere of the driving source, but may be formed instead at a standing shock near the basis of the jet and spatially detached from ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/m17_hh.pdf -- 1590.6 Кб -- 04.04.2013
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    83. http://www.eso.org/~fcomeron/g76.pdf
    ... However, observations have thus far revealed a handful of cases in which the photosphere of the central star can be directly observed (Watson & Hanson 1997, Feldt et al. ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/g76.pdf -- 618.1 Кб -- 10.06.2008
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    84. http://www.eso.org/~fpatat/science/sn06X/preprint.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, since they would cause variations in all absorption features ...
    [ Текст ]  Ссылки http://www.eso.org/~fpatat/science/sn06X/preprint.pdf -- 1998.7 Кб -- 18.07.2007
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    85. http://www.eso.org/~fcomeron/s106.pdf
    ... The 2MASS colors of S106 IR, ( J - H ) = 1.54, (H - KS ) = 1.08, are normal for an early stellar photosphere significantly reddened by foreground extinction. ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/s106.pdf -- 1474.6 Кб -- 10.06.2008
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    86. http://www.eso.org/~fcomeron/lup_c2d_spec.pdf
    ... claim of a numerous population of new members around Lupus 1, based on the statistics of stars fitted by a cool photosphere, is largely disproved by the available spectroscopy, which shows that over 80 % of the selected candidates observed are actually ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/lup_c2d_spec.pdf -- 1519.6 Кб -- 04.04.2013
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    87. http://www.eso.org/~fcomeron/rcw108-xray.pdf
    ... On the other hand, the K magnitudes of younger sources are brighter than their photosphere due to the contribution of disks. ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/rcw108-xray.pdf -- 2422.6 Кб -- 10.06.2008
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    88. http://www.eso.org/~mvandena/haebe_hi.ps.gz
    ... If the spectral resolution of the EW measurement is suфcient to discern the EW of the photosphere the H , the EW gives us a direct measure of the emission line. ...
    [ Текст ]  Ссылки http://www.eso.org/~mvandena/haebe_hi.ps.gz -- 235.7 Кб -- 03.09.2002
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    89. http://www.eso.org/~mvandena/pdrshock.ps.gz
    ... A fit consisting of the sum of a reddened Kurucz (1991) model for the stellar photosphere and a spline fitted to the ex­ cesses in the infrared to submm range, extrapolated to infinity by a blackbody curve, was made to the energy distribution for each ...
    [ Текст ]  Ссылки http://www.eso.org/~mvandena/pdrshock.ps.gz -- 375.7 Кб -- 03.09.2002
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    90. http://www.eso.org/~fcomeron/cygob2_ext.pdf
    ... Protostellar sources: two objects in our sample display ex- cal of a cold photosphere, except perhaps for its broader CO bands. ...
    [ Текст ]  Ссылки http://www.eso.org/~fcomeron/cygob2_ext.pdf -- 904.5 Кб -- 10.06.2008
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