THE CONFLUENT SYSTEM FORMALISM .2. THE GROWTH HISTORY OF OBJECTS

Citation
A. Manrique et E. Salvadorsole, THE CONFLUENT SYSTEM FORMALISM .2. THE GROWTH HISTORY OF OBJECTS, The Astrophysical journal, 467(2), 1996, pp. 504-521
Citations number
30
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
467
Issue
2
Year of publication
1996
Part
1
Pages
504 - 521
Database
ISI
SICI code
0004-637X(1996)467:2<504:TCSF.T>2.0.ZU;2-3
Abstract
We conclude the presentation of a semianalytical model of hierarchical clustering of bound virialized objects formed by gravitational instab ility from a random Gaussian field of density fluctuations. In the fir st paper of this series, we introduced the basic tool, the so-called c onfluent system formalism, able to follow the evolution of bound viria lized objects in the peak model. This was applied to derive the mass f unction of objects. In the present paper, we calculate other important quantities that characterize the growth history of objects. This mode l is compared with a similar one obtained by Lacey St. Cole following the Press-Schechter approach. The interest of the new modeling present ed here is twofold: (1) it is formally better justified, as far as pea ks are more reasonable seeds of objects than the undetermined regions in the Press-Schechter prescription, and (2) it distinguishes between merger and accretion, enabling us to unambiguously define the formatio n and destruction of objects and to estimate growth rates and characte ristic rimes not available in the previous approach.