Signs of gas flows in the variable Balmer line profiles of the Seyfert galaxy nuclei NGC 3227 and NGC 7469

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Table 1:

The compiled data for the NGC 3227.
Date	Aperture	Nucleus	Sy type	References
		brightness
1	2	3	4	5
03.1967	?	deep minim.	Sy2	1
01.1977	$1\hbox{$.\!\!^{\prime\prime}$ }0\times 1\hbox{$.\!\!^{\prime\prime}$ }5$	flare in max.	Sy1	2
01.1990	see Fig. 4	maximum	Sy1	3
01.1992	$5''\times 10''$	flare in max.	Sy1	4
03.1992	$5''\times 10''$	maximum	Sy1	4

References: 1 - Rubin, Ford (1968); 2 - Pronik, Metik (2004, 2005);
3 - Salamanka et al. (1994); 4 - Winge et al. (1995).

Source LaTeX | All tables | In the text

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