... From stellar synthesis they found that the corresponding stellar cluster is less than 1.6 Gyr old, and the bolometric luminosity of the cluster within 1 is at least 2.7 в 109 L . ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_425_77.pdf -- 483.6 Кб -- 24.02.2010 Похожие документы
... for the study of the properties of the Galactic disk including the history of star ... of M-type dwarfs in open clusters and calibrated the "ageactivity" relation ... 19.3 pc) and belongs to the galactic disk population, we can suppose that its metal ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2007/AstBu_62_117.pdf -- 558.2 Кб -- 24.02.2010 Похожие документы
... data for most of the systems: Galactic coordinates, maximum X-ray intensity, orbital ... systems, we give both 2 celestial and Galactic coordinates and the maximum X-ray ...
... 49. Goranskij V.P., Barsukova E.A. V79 in the globular cluster Messier 3 returns to fundamental mode. ... In "Variable stars, the Galactic halo and Galaxy formation". B.V.Kukarkin Centennary Conference. Ed. Chr. ...
... 49. Goranskij, V.P., Barsukova, E.A. V79 in the globular cluster Messier 3 returns to fundamental mode. ... In "Variable stars, the Galactic halo and Galaxy formation". B.V.Kukarkin Centennary Conference. Ed. Chr. ...
... extended ob ject (2 в4 ) outside the galactic plane, IRC +10 216 was the brightest ... evolved post-asymptotic giant branch (post-AGB) stars, and in active galactic nuclei ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_368_497M.pdf -- 1354.2 Кб -- 24.02.2010 Похожие документы