All Tables
- Table 1:
Summary of observations.
- Table 2:
Results of optical and near-infrared aperture photometry in Mkn 1087 and KPG 103a knots.
- Table 3:
General spectroscopic properties of the knots.
- Table 4:
Dereddened line intensity ratios with respect to I(H
) = 100 for the three brightest star-forming bursts observed in Mkn 1087: the center of Mkn 1087 (C), the north companion galaxy (N) and the intense burst #7. All have been observed both with 4.2 m WHT and 2.5 m INT. Correction for underlying stellar absorption in H I Balmer lines has been also applied.
- Table 5:
Dereddened line intensity ratios with respect to I(H
) = 100 for the faint knots observed in Mkn 1087. Correction for underlying stellar absorption in H I Balmer lines was also applied. All spectra were taken using INT.
- Table 6:
Chemical abundances of the knots.
- Table 7:
Structural parameters of Mkn 1087 and the brightest galaxies and objects associated with it.
- Table 8:
B-magnitude (not corrected by reddening) and (B-R) color of some of the background galaxies (bg) found in the area surrounding Mkn 1087. The objects belonging to the non-catalogued cluster (cl) show redder colors.