The very local Hubble flow: simulating the transition from chaos to order

被引：16

作者：

Chernin, A. D. ^{[1
]}

Karachentsev, I. D.

Valtonen, M. J.

Dolgachev, V. P.

Domozhilova, L. M.

Makarov, D. I.

机构：

[1] Turku Univ, Tuorla Observ, Piikkio 21500, Finland

[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia

[3] Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia

[4] Univ W Indies, St Augustine, Trinidad Tobago

[5] Isaac Newton Inst Chile, SAO Branch, Moscow, Russia

来源：

ASTRONOMY & ASTROPHYSICS | 2007年 / 467卷 / 03期

关键词：

galaxies : Local Group;

D O I：

10.1051/0004-6361:20053458

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The physical nature of the very local (< 3 Mpc) Hubble flow is studied on the basis of the recent high-precision observations in the Local Volume. A model including both analytical treatment and computer simulations describes the flow's dynamical evolution from a chaotic Little Bang initial state to the present-day state of a quasi-regular expansion. The dynamical effect of the uniform cosmic vacuum ( time-independent dark energy or the cosmological constant) is taken into account.

引用

收藏

页码：933 / 941

页数：9

相关论文

共 37 条

[1] The cold local Hubble flow as a signature of dark energy [J].

Baryshev, YV ;

Chernin, AD ;

Teerikorpi, P .

ASTRONOMY & ASTROPHYSICS, 2001, 378 (03) :729-734

[2] ORBITS OF THE MAGELLANIC CLOUDS AND LEO-I IN LOCAL GROUP HISTORY [J].

BYRD, G ;

VALTONEN, M ;

MCCALL, M ;

INNANEN, K .

ASTRONOMICAL JOURNAL, 1994, 107 (06) :2055-2059

[3] Why is the Hubble flow so quiet? [J].

Chernin, A ;

Teerikorpi, P ;

Baryshev, Y .

SMALL SATELLITES FOR ASTROPHYSICAL RESEARCH, THE COPERNICAN PRINCIPLE AND HOMOGENEITY OF THE UNIVERSE, 2003, 31 (02) :459-467

[4] Non-Friedmann cosmology for the Local Universe, significance of the universal Hubble constant, and short-distance indicators of dark energy [J].

Chernin, A. D. ;

Teerikorpi, P. ;

Baryshev, Yu. V. .

ASTRONOMY & ASTROPHYSICS, 2006, 456 (01) :13-21

[5]

Chernin A. D., 1998, New Astronomy Reviews, V42, P41, DOI 10.1016/S1387-6473(98)00021-9

[6] The very local Hubble flow: Computer simulations of dynamical history [J].

Chernin, AD ;

Karachentsev, ID ;

Valtonen, MJ ;

Dolgachev, VP ;

Domozhilova, LM ;

Makarov, DI .

ASTRONOMY & ASTROPHYSICS, 2004, 415 (01) :19-25

[7] Cosmic vacuum [J].

Chernin, AD .

PHYSICS-USPEKHI, 2001, 44 (11) :1099-1118

[8] Velocity and spatial biases in cold dark matter subhalo distributions [J].

Diemand, J ;

Moore, B ;

Stadel, J .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 352 (02) :535-546

[9] Galactic systems against the background of the cosmic vacuum: Structure and evolution of the zero-acceleration surface [J].

Dolgachev, VP ;

Domozhilova, LM ;

Chernin, AD .

ASTRONOMY REPORTS, 2004, 48 (10) :787-794

[10] The zero-acceleration surface around the local group of galaxies [J].

Dolgachev, VP ;

Domozhilova, LM ;

Chernin, AD .

ASTRONOMY REPORTS, 2003, 47 (09) :728-732

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