Using direct plates obtained at the prime focus of the 2.6-m telescope of the Byurakan Astrophysical Observatory (ZU-21 plates), we have investigated the central regions of ultraviolet galaxies. For seven galaxies, listed in Table 1, double nuclei have been found for the first time. The plates were analyzed using the PDS 1010A--CM4 densitometer complex by means of a program for analyzing extended objects in the framework of the ADA computational system of the Byurakan Astrophysical Observatory. The analysis included scanning the images of the galaxies with a 0:'5 diaphragm, surface photometry of the objects in the B system with construction of contour charts either in units of magnitudes per square second or in densities; estimate of the integrated magnitudes of the galaxies and the identified nuclei; estimate of the geometrical characteristics of the galaxies. The accuracy of the photometry, with transition to the B system, was estimated at +0.m19. We also give a brief description of the central parts of all the investigated galaxies, their isophotes, and geometrical sections through both nuclei. The galaxies for which a complex structure has been discovered for the first time are given in Table 1, which contains the Markaryan numbers of the galaxies, the absolute and apparent integrated magnitudes of the galaxies and their nuclei, the radial velocities (corrected for revolution of the sun, in accordance with [1]), the diameters of the galaxies in seconds of arc and in kiloparsecs, the distances between the components in seconds of arc and kiloparsecs, the apparent and absolute integrated magnitudes of the nuclei, which are designated as in [2], and the morphological types and spectral class according to [4, 5]. We determined the apparent magnitudes of the nuclei visually by the method described in [3]. Figure 1 gives isophote charts of the galaxies. The isophotes were constructed in magnitudes in the B filter per square second. There now follows a description of the galaxies in accordance with the photographs obtained with the 2.6-m telescope. Markaryan 1003. A barred spiral whose arms form a spherical ring. At least two condensations can be identified in the equatorial plane. The fainter condensation is at the geometrical center, and the brighter may be a giant H II region. Markaryan 1126. This is a Seyfert with two nuclei. There is a ring around the bulge. The galaxy has three envelopes. The inner isotopes are spherical, the outer have a cut form. Markaryan 1127. A spiral with faint arms. Within the innermost rectangular isophote at least two condensations are observed. There may be two more which we could not reliably identify but suspected in the photometric section. Markaryan 1131. A spiral galaxy with large bulge in which two nuclei can be identified. The bright nucleus is closer to the center of the galaxy. The second nucleus may be a giant H II region. Being faint, the second component is not clearly revealed in the isophote chart. Markaryan 1140. A barred spiral with two well-defined nuclei; its spiral arms are uniform. The nuclei are well revealed in the photometric section. Markaryan 1156. A somewhat elongated two-nucleus galaxy with weakly developed spiral arms. The nuclei differ strongly in brightness, and neither is at the geometrical center of the galaxy. The outer isophotes are strongly cut. It is possible that the first nucleus is itself divided into two components. Markaryan 1187. This is a Seyfert. In the center there are two nuclei that do not differ strongly in brightness. All the isophotes, the outer and the inner, are very cut. The morphological type is SBc.
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