Evidence to disfavour dual core system leading to double-peaked narrow emission lines

In this manuscript, an interesting method is proposed to test dual core system for double-peaked narrow emission lines, through precious dual core system with double-peaked narrow Balmer lines in one system in main galaxy but with single-peaked narrow Balmer lines in the other system in companion galaxy. Under a dual core system, considering narrow Balmer (H$\alpha$ and H$\beta$) emissions ($f_{e,\alpha }$ and $f_{e,\beta }$) from companion galaxy but covered by SDSS fiber for the main galaxy and narrow Balmer emissions ($f_{c,\alpha }$ and $f_{c,\beta }$) from the companion galaxy covered by SDSS fiber for the companion galaxy, the same flux ratios $f_{e,\alpha }\mathrm{/}{f}_{c,\alpha }=f_{e,\beta }\mathrm{/}{f}_{c,\beta }$ can be expected, due to totally similar physical conditions of each narrow Balmer emission region. Then, the precious dual core system in SDSS J2219-0938 is discussed. After subtracting pPXF code determined stellar lights, double-peaked narrow Balmer emission lines are confirmed in the main galaxy with confidence level higher than $5\sigma$, but single-peaked narrow Balmer emission lines in the companion galaxy. Through measured fluxes of emission components, $f_{e,\alpha }\mathrm{/}{f}_{c,\alpha }$ is around 0.82, different from $f_{e,\beta }\mathrm{/}{f}_{c,\beta }\sim 0.52$, to disfavour a dual core system for the double-peaked narrow Balmer emission lines in SDSS J2219-0938.