Physical characteristics of the nucleus of the galaxy Markaryan 6

Astrophysics ◽  
1975 ◽  
Vol 9 (1) ◽  
pp. 76-78
Author(s):  
�. E. Khachikyan
Keyword(s):  
Physical Characteristics ◽  
The Galaxy ◽  
Galaxy Markaryan

Spectrophotometry of the galaxy Markaryan 266

Astrophysics ◽  
1981 ◽  
Vol 16 (4) ◽  
pp. 366-374 ◽  
Author(s):  
A. R. Petrosyan
Keyword(s):  
The Galaxy ◽  
Galaxy Markaryan

Hydrogen lines in the spectrum of the galaxy Markaryan 6 during its activity

Astrophysics ◽  
1974 ◽  
Vol 8 (2) ◽  
pp. 112-116 ◽  
Author(s):  
V. I. Pronik ◽  
K. K. Chuvaev
Keyword(s):  
The Galaxy ◽  
Hydrogen Lines ◽  
Galaxy Markaryan

Spectral investigation of the galaxy Markaryan 297

Astrophysics ◽  
1988 ◽  
Vol 28 (1) ◽  
pp. 26-34
Author(s):  
A. N. Burenkov
Keyword(s):  
Spectral Investigation ◽  
The Galaxy ◽  
Galaxy Markaryan

Spectral investigation of the galaxy Markaryan 8

Astrophysics ◽  
1974 ◽  
Vol 8 (4) ◽  
pp. 311-316
Author(s):  
�. E. Khachikyan
Keyword(s):  
Spectral Investigation ◽  
The Galaxy ◽  
Galaxy Markaryan

Radio emission of the galaxy Markaryan 668 in the frequency range 2.3?14.4 GHz

Astrophysics ◽  
1979 ◽  
Vol 14 (4) ◽  
pp. 390-392
Author(s):  
V. A. Sanamyan ◽  
R. A. Kandalyan
Keyword(s):  
Radio Emission ◽  
Frequency Range ◽  
The Galaxy ◽  
Galaxy Markaryan

Detailed morphological and spectrophotometric investigation of the galaxy Markaryan 1118

Astrophysics ◽  
1989 ◽  
Vol 29 (2) ◽  
pp. 537-542
Author(s):  
A. N. Burenkov ◽  
A. R. Petrosyan ◽  
A. B. Sarkisyan ◽  
�. E. Khachikyan
Keyword(s):  
Spectrophotometric Investigation ◽  
The Galaxy ◽  
Galaxy Markaryan

Spectral investigation of the galaxy markaryan 111

Astrophysics ◽  
1984 ◽  
Vol 21 (3) ◽  
pp. 588-595
Author(s):  
A. N. Burenkov ◽  
A. R. Petrosyan ◽  
K. A. Saakyan ◽  
É. E. Khachikyan
Keyword(s):  
Spectral Investigation ◽  
The Galaxy ◽  
Galaxy Markaryan

scholarly journals A Linkup Between Seyfert's and their Surroundings

1996 ◽  
Vol 171 ◽  
pp. 408-408
Author(s):  
A.P. Mahtessian ◽  
E.Ye. Khachikian ◽  
H. Tiersch
Keyword(s):  
Seyfert Galaxies ◽  
Physical Characteristics ◽  
Active Galaxies ◽  
Galaxy Groups ◽  
The Galaxy ◽  
Redshift Survey ◽  
Insight Into

The observed physical characteristics of galaxies are (at least partly) determined by the influence of the surroundings after the formation of the galaxies. The examination of the frequency of the occurence of active galaxies, i.e. Seyfert galaxies, in different galaxy systems compared to a sample of field galaxies gives possibly an insight into this problem.The galaxy groups were taken from the CfA redshift survey, the list of them is published in Mahtessian (1992, Soob. Byurakan. Obs. 65).

scholarly journals A Semi-Analytic Approach to Understanding the Bimodality of GCs in the Milky Way & M31

2006 ◽  
Vol 2 (S235) ◽  
pp. 132-132
Author(s):  
B. Rothberg ◽  
R. Somerville ◽  
B. Whitmore ◽  
W. Harris
Keyword(s):  
Globular Clusters ◽  
Milky Way ◽  
Spiral Galaxies ◽  
Broad Band ◽  
Physical Characteristics ◽  
Analytic Approach ◽  
The Galaxy ◽  
Analytic Models ◽  
Parent Galaxy ◽  
Centaurus A

AbstractOne of the most important results in the study of Globular Clusters (GC) has been the discovery of bimodality in the broad-band colors of many systems. Observations of the Milky Way, M31 and Centaurus A strongly suggest this is a bi-modality in metallicity. One method of constraining, and perhaps better understanding the observed bimodality of GCs is to use semi-analytic models (SAMs) to test both the galaxy and GC formation scenarios. We present the results of a study to test whether SAMs can accurately reproduce the physical characteristics of both the parent galaxy (including luminosity, mass and metallicity) and GC populations. The focus of the work is to test whether the SAMs are capable of reproducing the observed properties of spiral galaxies, in particular the Milky Way and M31, and what, if any, constraints this may place on the formation scenarios of GCs. Among the results are indications that bimodality may be directly connected with reionization at z ~ 7–8.

Spectroscopic observations of the galaxy Markaryan 6

Astrophysics ◽  
1975 ◽  
Vol 9 (1) ◽  
pp. 20-25
Author(s):  
P. Notni ◽  
�. E. Khachikyan ◽  
M. M. Butslov ◽  
G. G. Gevorkyan
Keyword(s):  
Spectroscopic Observations ◽  
The Galaxy ◽  
Galaxy Markaryan
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