Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.sao.ru/precise/Laboratory/Publications/1997/CasePR/node8.html
Дата изменения: Sat Jan 10 17:37:56 1998
Дата индексирования: Sat Sep 11 20:37:09 2010
Кодировка:

Поисковые слова: m 42
Quasar CG 273 next up previous
Next: Preliminary analysis of the Up: Results of observations Previous: The main observational parameters

Quasar CG 273

One of the Case galaxies appeared to be a distant and bright AGN. This is CG 273 ($\alpha$= 09h39m05s.8, $\delta$= +35$^{\circ}$36'42", mCG=18 mag). Only one prominent emission line is seen in the wavelength range 3600 - 5500 Å. This broad emission line is centered at $\lambda$4673 Å and its FWHM is 50 Å. We identify it with the MgII doublet $\lambda$2798 Å, the corresponding redshift is 0.670. With the Hubble constant 75 km s-1Mpc-1 and q0=0.5 its absolute blue magnitude MB= -25 mag, which places CG 273 to the class of quasars. We show its spectrum in Fig. 1.



root
1/10/1998