Title of article :
YOU CANT GET THERE FROM HERE: HUBBLE RELAXATION IN THE LOCAL VOLUME
Author/Authors :
WHITING، ALAN B. نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2006
Pages :
-1995
From page :
1996
To page :
0
Abstract :
A beginning endpoint for galaxy motions within the 10 Mpc Local Volume is constructed by requiring a smooth distribution of (luminous) matter at the time of recombination, which is shown to be equivalent to a smooth Hubble flow at early times. It is found, by this purely kinematical method, that present peculiar motions are too small by a factor of at least several (and largely in the wrong direction) to have produced the observed structures within the age of the universe. Known dynamical effects are inadequate to remove the discrepancy. This result is different in origin from previously known "cold flow" problems. The simple dynamical picture often used within the Local Volume (for instance, in deriving masses through calculation of a zero-velocity surface) is thus called into question. The most straightforward explanation (although not the only possible) is that there exists a large quantity of baryonic matter in this region so far undetected, and unassociated with galaxies or groups.
Keywords :
large-scale structure of universe , galaxies: kinematics and dynamics
Journal title :
Astronomical Journal
Serial Year :
2006
Journal title :
Astronomical Journal
Record number :
116774
Link To Document :
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