... gzipped) PostScript (203 KB) . RX J0529.8-6556: a new pulsating Be/X-ray transient in the LMC . F. Haberl, K. Dennerl, W. Pietsch, and K. Reinsch . ...
... the supernova remnant N132D is imaged in the light of [O III] 5007е against a background of ~104 stars in the bar of the LMC ... veloc subtracted images go far deeper than conventional narrow-band imag the LMC in the light of [O III] 5007е telescope ...
[
Текст
]
Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/NICFPS/OLD/NICFPS_projdescr.pdf -- 2005.8 Кб -- 06.09.2002 Похожие документы
... With incredible foresight, these experimentalists completed in late 1986 their revisions to make the detector sensitive to solar neutrinos, just in time to observe the neutrinos from Supernova 1987a emitted in the LMC 170,000 years earlier. ...
... Note that NGC 1466 is a globular cluster (not a galaxy) between the LMC and the SMC; we presented it separately, because it is not clear to which galaxy to attribute its variable stars. ...
... Relative frequencies of Type Ia and Type II supernovae in the chemical evolution of the Galaxy, LMC and SMC / T. Tsujimoto, K. Nomoto, Y. Yoshii et al. ...
[
Текст
]
Ссылки http://www.inasan.rssi.ru/~kurbatov/Kurbatov--2010phdt.nmceg.pdf -- 544.7 Кб -- 06.09.2012 Похожие документы
... projected distance between the two galaxies is only 20 , or 50 kpc; it is comparable to the distance between our Galaxy and the LMC, and considering the existence of the Magellanic Stream, we would expect tidal interaction between NGC 3623 and NGC 3627 ...
... B1b. The viscosity of the mixture is calculated as a product of the meltcrystal viscosity and the relative viscosity due to the presence of bubble phase. l ј lmc Пc; T ; bчlr ПCa; aч References Ambler, E.P., Ashley, P.M., 1977. ...
[
Текст
]
Ссылки http://geo.web.ru/users/pavel/Publications/2006/Dirksen06.pdf -- 1392.8 Кб -- 16.01.2008 Похожие документы