Tilted cold dark matter models confront the cosmic microwave background and the galaxy peculiar velocity field

1993 ◽  
Vol 410 ◽  
pp. L61 ◽  
Author(s):  
Pio F. Muciaccia ◽  
Simona Mei ◽  
Giancarlo de Gasperis ◽  
Nicola Vittorio
1993 ◽  
Vol 411 ◽  
pp. 16 ◽  
Author(s):  
Giuseppe Tormen ◽  
Lauro Moscardini ◽  
Francesco Lucchin ◽  
Sabino Matarrese

1991 ◽  
Vol 372 ◽  
pp. L1 ◽  
Author(s):  
Nicola Vittorio ◽  
Peter Meinhold ◽  
Philip Lubin ◽  
Pio Francesco Muciaccia ◽  
Joseph Silk

1990 ◽  
Vol 124 ◽  
pp. 645-649
Author(s):  
Tetsuya Hara ◽  
Shigeru Miyoshi

It has been reported that galaxies in large regions (~102Mpc), including some clusters of galaxies, may be streaming coherently with velocities up to 600km/sec or more with respect to the rest frame determined by the microwave background radiation.) On the other hand, it is suggested that the dominant mass component of the universe is dark matter. Because we can only speculate the motion of dark matter from the galaxy motions, much attention should be paid to the correlation of velocities between the observed galaxies and cold dark matter. So we investigate whether such coherent large-scale streaming velocities are due to dark matter or only to baryonic objects which may be formed by piling up of gases due to some explosive events.


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