You Can't Get There From Here: Hubble Relaxation in the Local Volume
Author(s) -
Alan B. Whiting
Publication year - 2006
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/500580
Subject(s) - physics , galaxy , flow (mathematics) , astrophysics , hubble volume , universe , baryon , hubble's law , theoretical physics , classical mechanics , statistical physics , redshift , mechanics
A beginning end-point for galaxy motions within the 10-Mpc Local Volume isconstructed by requiring a smooth distribution of (luminous) mass at the timeof recombination, which is shown to be equivalent to a smooth Hubble flow atearly times. It is found, by this purely kinematical method, that presentpeculiar motions are too small by a factor of at least several (and largely inthe wrong direction) to have produced the observed structures within the age ofthe 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 (forinstance, in deriving masses through calculation of a zero-velocity surface) isthus called into question. The most straightforward explanation (though not theonly possible) is that there exists a large quantity of baryonic matter in thisregion so far undetected, and unassociated with galaxies or groups.Comment: 23 pages, accepted by the Astronomical Journa
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