... es jusqu'aux derniРеres limites, le diamРеtre apparent d'un grand nombre d'Р?toiles put Р?tre rigoureusement mesurР?, et M. Clarke, du bureau de Cambridge, dР?composa le crabnebula * du Taureau, que le rР?flecteur de Lord Rosse n'avait jamais pu rР?duire ...
... line of neutral hydrogen in the interstellar medium together with some molecular radio lines; explanation of the spectrum of the CrabNebula in the optical and radio ranges by a unified synchrotron mechanism; his works on the radio emission of the solar ...
... They were predicted theoreticallyby Landau [1] in the early 1930s, and the first radio pulsar was found in the center of the Crabnebula in the early 1960s. At the beginning of the 1970s--an epoch of active programs in near-Earth space exploration--the ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/NS_OBgiants_eng.pdf -- 331.6 Кб -- 11.02.2004 Похожие документы
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... The maximum X-ray brightness at 212 keV was 2 Crabs, and was achieved on April 1 at 0h 57m UT (JD 2450904.54). ... According to [13], it may still be possible to explain the radio nebula as the product of ASTRONOMY REPORTS Vol. ...