NGC 6946 galaxy BH Mass ~ M 0.95 bulge.

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Presentation transcript:

NGC 6946 galaxy

BH Mass ~ M 0.95 bulge

BH Mass ~ σ 4

open circles – high-mass bulge galaxies filled circles – low-mass bulge galaxies

Fig. 16. MACHO-98-BLG-06 microlensing light curve (D.P.Bennett et al., 2002)

Fig. 19. Light curves due to microlensing of a star by a wormhole for different impact parameters: p=2.1  E, 1.9  E, 1.0  E, and 0

Fig.20. Changes of polarization degree during microlensing of a star by a wormhole

A.Fletcher et al., A&A, 414, (2004)

astro-ph/ , Pulsar rotation measures and the large-scale structure of Galactic magnetic field J.L.Han, R.N.Manchester, A.G.Lyne, G.J.Qiao, W.van Straten, Astrophys.J. 642, , 2006.

Двойная система – два входа в магнитный тоннель N S

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Первичные магнитные кротовые норы в «Многомире» («Multiverse»)

Параметры кротовых нор

Двойные системы входов в магнитный тоннель

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Учёные из Италии предположили, что Вселенная может иметь вытянутую, а не правильную сферическую, форму. Вселенная могла растянуться в элипсоид под действием магнитного поля, распределенного по ней, или из-за дефектов в структуре пространства-времени. Предположение было сделано на основе данных, собранных космическим аппаратом NASA WMAP.

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3C273

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A View through Faraday's Fog: Parsec-Scale Rotation Measures in Active Galactic Nuclei, Zavala, R. T.; Taylor, G. B., The Astrophysical Journal, V. 589, pp , BL Lac, z=0.07, F 15 =3.23 Jy.