Further evidence for an explosive event in the peculiar galaxy NGC 1569

1974 ◽  
Vol 194 ◽  
pp. L119 ◽  
Author(s):  
G. de Vaucouleurs ◽  
A. de Vaucouleurs ◽  
W. Pence
Keyword(s):  
Peculiar Galaxy ◽  
Explosive Event ◽  
Ngc 1569

scholarly journals The peculiar galaxy IC 1182: An ongoing merger?

2004 ◽  
Vol 418 (2) ◽  
pp. 495-507 ◽  
Author(s):  
M. Moles ◽  
D. Bettoni ◽  
G. Fasano ◽  
P. Kjærgaard ◽  
J. Varela ◽  
...  
Keyword(s):  
Peculiar Galaxy

FISICA observations of the starburst galaxy, NGC 1569

2006 ◽  
Vol 50 (4-5) ◽  
pp. 433-435
Author(s):  
D.M. Clark ◽  
S.S. Eikenberry ◽  
S.N. Raines ◽  
N. Gruel ◽  
R. Elston ◽  
...  
Keyword(s):  
Starburst Galaxy ◽  
Ngc 1569

scholarly journals ATCA HI observations of the peculiar galaxy IC 2554

2003 ◽  
Vol 339 (4) ◽  
pp. 1203-1222 ◽  
Author(s):  
Bärbel Koribalski ◽  
Scott Gordon ◽  
Keith Jones
Keyword(s):  
Peculiar Galaxy

Polarization investigation of the peculiar galaxy NGC 660

Astrophysics ◽  
1992 ◽  
Vol 35 (1) ◽  
pp. 285-287
Author(s):  
V. P. Reshetnikov ◽  
V. A. Yakovleva
Keyword(s):  
Peculiar Galaxy ◽  
Polarization Investigation

scholarly journals New Data on the Peculiar Galaxy MRK 273

1990 ◽  
Vol 124 ◽  
pp. 201-208 ◽  
Author(s):  
A. S. Asatrian ◽  
A. R. Petrosian ◽  
F. Börngen
Keyword(s):  
Radio Continuum ◽  
Main Body ◽  
Blue Color ◽  
Close System ◽  
Peculiar Galaxy ◽  
The Galaxy ◽  
Thermal Origin ◽  
Absorption Features

AbstractOn the basis of direct UBV and spectral observations at Tautenburg (DDR) 2m and Special Observatory (USSR) 6m telescopes respectively the colorimetric and spectral investigations of the megamaser galaxy MRK 273 are carried out. It is seen that: MRK 273 is in a physical group of galaxies, which contains at least five members. Two bright central condensations of MRK 273 are Seyfert nuclei. The area of the main body of MRK 273 which contains both Seyfert nuclei and from which comes out a straight tail, is redder than the remaining part of the galaxy. The tail has a pronounced blue color and most probably radiates in [OIII] λ5007 line. Observed radio continuum, OH and HI absorption features are related to bright “a” nucleus of galaxy. We come to the conclusion that MRK 273 which is the member of the group of the galaxies is itself a close system of two objects with AGNs. The tail, with radiation being of thermal origin, probably is the result of the interaction of these galaxies.

IR observations of the peculiar galaxy Arp220

Nature ◽  
1984 ◽  
Vol 311 (5983) ◽  
pp. 237-238 ◽  
Author(s):  
J. P. Emerson ◽  
P. E. Clegg ◽  
G. Gee ◽  
C. T. Cunningham ◽  
M. J. Griffin ◽  
...  
Keyword(s):  
Peculiar Galaxy

Spectroscopic study of the peculiar galaxy UGC 5119

2008 ◽  
Vol 34 (8) ◽  
pp. 542-550 ◽  
Author(s):  
O. A. Merkulova ◽  
L. V. Shalyapina ◽  
V. A. Yakovleva ◽  
G. M. Karataeva
Keyword(s):  
Spectroscopic Study ◽  
Peculiar Galaxy
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