Geodesic
Connection between morphological types and $SM$-properties of galaxies with $UV$-excess
Proceedings of the Yerevan State University. Physical and mathematical sciences, no. 3 (2008), pp. 76-81 
M. A. Kazarian; J. R. Martirosian. Connection between morphological types and $SM$-properties of galaxies with $UV$-excess. Proceedings of the Yerevan State University. Physical and mathematical sciences, no. 3 (2008), pp. 76-81. http://geodesic.mathdoc.fr/item/UZERU_2008_3_a10/
@article{UZERU_2008_3_a10,
     author = {M. A. Kazarian and J. R. Martirosian},
     title = {Connection between morphological types and $SM$-properties of galaxies with $UV$-excess},
     journal = {Proceedings of the Yerevan State University. Physical and mathematical sciences},
     pages = {76--81},
     year = {2008},
     number = {3},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/UZERU_2008_3_a10/}
}
TY  - JOUR
AU  - M. A. Kazarian
AU  - J. R. Martirosian
TI  - Connection between morphological types and $SM$-properties of galaxies with $UV$-excess
JO  - Proceedings of the Yerevan State University. Physical and mathematical sciences
PY  - 2008
SP  - 76
EP  - 81
IS  - 3
UR  - http://geodesic.mathdoc.fr/item/UZERU_2008_3_a10/
LA  - ru
ID  - UZERU_2008_3_a10
ER  - 
%0 Journal Article
%A M. A. Kazarian
%A J. R. Martirosian
%T Connection between morphological types and $SM$-properties of galaxies with $UV$-excess
%J Proceedings of the Yerevan State University. Physical and mathematical sciences
%D 2008
%P 76-81
%N 3
%U http://geodesic.mathdoc.fr/item/UZERU_2008_3_a10/
%G ru
%F UZERU_2008_3_a10

Voir la notice de l'article provenant de la source Math-Net.Ru

The correlation between morphological types and spectral-morphological ($SM$) properties of galaxies with $UV$-excess was found. The distribution of mean geometrical angular diameters of galaxies by the morphological types was determined. It is shown if mean geometrical diameters of galaxies are increased then relatively quantity of spectral morphology $d$ is increased. By the same rate of $UV$-excess radiation intensity the grouping morphological classes of galaxies are as follows: $St+C, E+Sph, S+L$ and $Ir$. It is found that $m_{pg}/''$ and $m_J/''$ with high $UV$-excess is more than the same value for galaxies with low $UV$-excess, except $m_{pg}/''$ in group $E+Sph$. It is also shown, that $m_{pg}/''$ and $m_J/''$ of galaxies with a spectra morphology of type $s+sd+ds$ is more than that for type $d$.

[1] M. A. Kazarian, “New Galaxies with UV Excess. I”, Astrophysics, 15 (1979), 1–15

[2] M. A. Kazarian, “New Galaxies with UV Excess. II”, Astrophysics, 15 (1979), 117–129

[3] M. A. Kazarian, “New Galaxies with UV Excess. III”, Astrophysics, 16 (1980), 7–20

[4] M. A. Kazarian, E. S. Kazaryan, “New Galaxies with UV Excess. IV”, Astrophysics, 18 (1982), 285–296

[5] M. A. Kazarian, E. S. Kazaryan, “New Galaxies with UV Excess. V”, Astrophysics, 19 (1982), 119–128

[6] M. A. Kazarian, G. V. Petrosian, “New Galaxies with UV Excess. VI”, Astrophysics, 48 (2005), 344–354

[7] M. A. Kazaryan, “Morfologicheskaya klassifikatsiya novykh galaktik s UF-izbytkom”, DOI: 10.1007/BF02071998, Astrofizika, 39 (1996), 431–440

[8] B. E. Markaryan, “Galaktiki s ultrafioletovym kontinuumom. I”, Astrofizika, 3 (1967), 55–68

[9] B. E. Markaryan, “Galaktiki s ultrafioletovym kontinuumom. II”, Astrofizika, 5 (1969), 443

[10] M. A. Kazaryan, Zh.R. Martirosyan, “Fizicheskaya svyaz galaktik Kazaryana s okruzhayuschimi galaktikami”, Astrofizika, 46 (2003), 207–220

[11] M. F. Skrutskie, R. M. Cutri, R. Stieninget all, “The Two Micron All Sky Survey (2MASS)”, The Astronomical Journal, 131 (2006), 1163–1183 | DOI