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221. http://www.stecf.org/conferences/adass/adassVII/reprints/polubekg.ps.gz
... Proximity e#ects of com ponents (reflection of radiation and surface gravity darkening) are taken into account. ... As an example, we consider the Algol (# Persei) system, where an eclipsing pair (Algol AB) is accompanied by the third component (Algol C). ... The surface temperature distribution for Algol AB system before (upper plot) and after (lower plot) correction for temperature due to the irradiation e#ect. ... We solve this equation by the iterative NewtonRaphson method. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/polubekg.ps.gz -- 194.4 Кб -- 12.06.2006
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222. http://www.armaghplanet.com/pdf/Administration/Approved%20Version%20AOP%20Business%20Plan%20201516.pdf
Version 1.0 Armagh Observatory and Planetarium Business Plan 2015/16 1 Version 1.0 Contents 1. ... 16 2 Version 1.0 1. ... The Armagh Observatory is the oldest scientific institution in Northern Ireland and the longest continuously operating astronomical research institute in the UK and Ireland. ... The Governors of the Armagh Observatory and Planetarium is a statutory corporation that operates under the authority of the Armagh Observatory and Planetarium (Northern Ireland) Order 1995. ...
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Ссылки http://www.armaghplanet.com/pdf/Administration/Approved%20Version%20AOP%20Business%20Plan%20201516.pdf -- 597.3 Кб -- 16.07.2015
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223. http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf
... Properties of Stellar Populations in Isolated Lenticular Galaxies I. Yu. ... The resulting average ages of the stellar population in bulges and discs fill an entire range of possible values from 1.5 to 15 Gyr which indicates the absence in the isolated lenticular galaxies, unlike in the members of groups and clusters, of a certain epoch when the structural components are formed: they could have been formed at a redshift of z > 2 as well as only several billion years ago. ... 69 NGC 2350 No. ...
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Ссылки http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf -- 1591.8 Кб -- 11.07.2015
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224. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
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Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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