The great attractor and the COBE quadrupole

2008 ◽  
pp. 304-304
Author(s):  
M. J. Fullana ◽  
D. P. Sáez ◽  
J. V. Arnau
Keyword(s):  
Great Attractor

scholarly journals Large-Scale Flows in the Local Universe

1996 ◽  
Vol 168 ◽  
pp. 175-182 ◽  
Author(s):  
D.S. Mathewson ◽  
V.L. Ford
Keyword(s):  
Large Scale ◽  
Velocity Measurements ◽  
Local Universe ◽  
Peculiar Velocities ◽  
Redshift Surveys ◽  
Density Maps ◽  
The Universe ◽  
Great Wall ◽  
Great Attractor ◽  
Streaming Flow

Peculiar velocity measurements of 2500 southern spiral galaxies show large-scale flows in the direction of the Hydra-Centaurus clusters which fully participate in the flow themselves. The flow is not uniform over this region and seems to be associated with the denser regions which participate in the flow of amplitude about 400km/s. In the less dense regions the flow is small or non-existent. This makes the flow quite asymmetric and inconsistent with that expected from large-scale, parallel streaming flow that includes all galaxies out to 6000km/s as previously thought. The flow cannot be modelled by a Great Attractor at 4300km/s or the Centaurus clusters at 3500km/s. Indeed, from the density maps derived from the redshift surveys of “optical” and IRAS galaxies, it is difficult to see how the mass concentrations can be responsible particularly as they themselves participate in the flow. These results bring into question the generally accepted reason for the peculiar velocities of galaxies that they arise solely as a consequence of infall into the dense regions of the universe. To the N. of the Great Attractor region, the flow increases and shows no sign of diminishing out to the redshift limit of 8000km/s in this direction. We may have detected flow in the nearest section of the Great Wall.

scholarly journals CAN GENERAL RELATIVISTIC DESCRIPTION OF GRAVITATION BE CONSIDERED COMPLETE?

1998 ◽  
Vol 13 (17) ◽  
pp. 1393-1400 ◽  
Author(s):  
D. V. AHLUWALIA
Keyword(s):  
Solar System ◽  
Gravitational Potential ◽  
Invariance Properties ◽  
Planetary Orbits ◽  
Galactic Cluster ◽  
General Relativistic ◽  
Relativistic Description ◽  
Flavor Oscillation ◽  
Weak Fields ◽  
Great Attractor

The local galactic cluster, the Great attractor, embeds us in a dimensionless gravitational potential of about -3×10-5. In the solar system, this potential is constant to about 1 part in 1011. Consequently, planetary orbits, which are determined by the gradient in the gravitational potential, remain unaffected. However, this is not so for the recently introduced flavor-oscillation clocks where the new redshift-inducing phases depend on the gravitational potential itself. On these grounds, and by studying the invariance properties of the gravitational phenomenon in the weak fields, we argue that there exists an element of incompleteness in the general relativistic description of gravitation. An incompleteness-establishing inequality is derived and an experiment is outlined to test the thesis presented.

A Survey in the Direction of the Great Attractor

1997 ◽  
pp. 299-301
Author(s):  
Ron Hola ◽  
Matthew Colless ◽  
Bruce A. Peterson ◽  
Somak Raychaudhury
Keyword(s):  
Great Attractor

Looking Well beyond the Great Attractor

Science News ◽  
1989 ◽  
Vol 135 (15) ◽  
pp. 230
Author(s):  
I. Peterson
Keyword(s):  
Great Attractor

A search for X-ray emission associated with the great attractor

1989 ◽  
Vol 346 ◽  
pp. 638 ◽  
Author(s):  
Keith Jahoda ◽  
Richard F. Mushotzky
Keyword(s):  
X Ray ◽  
Great Attractor

scholarly journals Near-infrared study of CIZA J1324.7-5736, the second richest cluster of galaxies in the Great Attractor

2006 ◽  
Vol 368 (2) ◽  
pp. 534-543 ◽  
Author(s):  
T. Nagayama ◽  
P. A. Woudt ◽  
K. Wakamatsu ◽  
S. Nishiyama ◽  
C. Nagashima ◽  
...  
Keyword(s):  
Near Infrared ◽  
Infrared Study ◽  
Cluster Of Galaxies ◽  
Great Attractor

AGNs, X-ray background and the possible candidates for great attractor

1990 ◽  
Vol 171 (1-2) ◽  
pp. 43-47
Author(s):  
J. M. Mart�n-Mirones ◽  
L. J. Goicoechea
Keyword(s):  
X Ray ◽  
X Ray Background ◽  
Great Attractor

scholarly journals Mapping the Hidden Universe: The Galaxy Distribution in the Zone of Avoidance

2000 ◽  
Vol 17 (1) ◽  
pp. 6-12 ◽  
Author(s):  
Renée C. Kraan-Korteweg ◽  
Sebastian Juraszek
Keyword(s):  
Milky Way ◽  
Current Status ◽  
Microwave Background ◽  
Galaxy Distribution ◽  
Velocity Flow ◽  
The Galaxy ◽  
The Mean ◽  
Zone Of Avoidance ◽  
Mean Time ◽  
Great Attractor

AbstractDue to the foreground extinction of the Milky Way, galaxies become increasingly faint as they approach the Galactic Equator creating a ‘zone of avoidance’ (ZOA) in the distribution of optically visible galaxies of about 25%. A ‘whole-sky’ map of galaxies is essential, however, for understanding the dynamics in our local Universe, in particular the peculiar velocity of the Local Group with respect to the Cosmic Microwave Background and velocity flow fields such as in the Great Attractor (GA) region. The current status of deep optical galaxy searches behind the Milky Way and their completeness as a function of foreground extinction will be reviewed. It has been shown that these surveys—which in the mean time cover the whole ZOA (Figure 2)—result in a considerable reduction of the ZOA from extinction levels of AB =1m.0 (Figure 1) to AB =3m.0 (Figure 3). In the remaining, optically opaque ZOA, systematic HI surveys are powerful in uncovering galaxies, as is demonstrated for the GA region with data from the full sensitivity Parkes Multibeam HI survey (300°≤l≤332°, ∣b∣≤5°.5, Figure 4).

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