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NGC 7579


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Determination of the relative spectrophotometric gradients of galaxies. IV
Relative spectrophotometric gradients of continua are determined for 195galaxies. The spectra have been obtained with the 70-cm meniscustelescope of the Abastumani Astrophysical Observatory using a 2-degpreobjective prism (the reverse linear dispersion was 1200 A/mm inH-gamma). The gradient values were reduced to the AO spectral class andcorrected for light absorption in the Galaxy.

Luminosity and mass models for the barred spiral galaxies NGC 7741, NGC 3359 and NGC 7479
From two-dimensional photometric data and the radial velocity field ofthe ionized gas, luminosity distributions and mass models of threelate-type barred spiral galaxies, NGC 7741, NGC 3359, and NGC 7479, areobtained. It is shown that the isoradial velocities clearly exhibit theclassical S-shaped distortion, expected from the gravitational pull ofthe bar. The near equality of the mass/luminosity ratios of the stellarbar and its surrounding disk is seen for the first two galaxies, but asignificantly lower value is seen for NGC 7479.

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Observation and Astrometry data

Constellation:Pegasus
Right ascension:23h17m38.90s
Declination:+09°26'00.0"
Aparent dimensions:0.457′ × 0.347′

Catalogs and designations:
Proper Names   (Edit)
NGC 2000.0NGC 7579
HYPERLEDA-IPGC 70963

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