The very local Hubble flow: Computer simulations of dynamical history

被引：42

作者：

Chernin, AD ^{[1
]}

Karachentsev, ID

Valtonen, MJ

Dolgachev, VP

Domozhilova, LM

Makarov, DI

机构：

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

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

[3] Univ Oulu, Astron Div, Oulu 90014, Finland

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

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

[6] Isaac Newton Inst Chile, SAO Branch, St Petersburg, Russia

来源：

ASTRONOMY & ASTROPHYSICS | 2004年 / 415卷 / 01期

关键词：

galaxies : Local Group;

D O I：

10.1051/0004-6361:20034170

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The phenomenon of the very local ( less than or equal to 3 Mpc) Hubble flow is studied on the basis of the data of recent precision observations. A set of computer simulations is performed to trace the trajectories of the flow galaxies back in time to the epoch of the formation of the Local Group. It is found that the "initial conditions" of the flow are drastically different from the linear velocity-distance relation. The simulations enable one also to recognize the major trends of the flow evolution and identify the dynamical role of universal antigravity produced by the cosmic vacuum.

引用

页码：19 / 25

页数：7

共 18 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] Cosmic vacuum [J].

Chernin, AD .

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

[5]

CHERNIN AD, 2003, ASTROPH0304250

[6] INTERGALACTIC MATTER AND THE GALAXY [J].

KAHN, FD ;

WOLTJER, L .

ASTROPHYSICAL JOURNAL, 1959, 130 (03) :705-717

[7] Hubble Space Telescope photometry of the dwarf spheroidal galaxy ESO 410-G005 [J].

Karachentsev, ID ;

Sharina, ME ;

Grebel, EK ;

Dolphin, AE ;

Geisler, D ;

Guhathakurta, P ;

Hodge, PW ;

Karachentseva, VE ;

Sarajedini, A ;

Seitzer, P .

ASTROPHYSICAL JOURNAL, 2000, 542 (01) :128-136

[8] The very local Hubble flow [J].

Karachentsev, ID ;

Sharina, ME ;

Makarov, DI ;

Dolphin, AE ;

Grebel, EK ;

Geisler, D ;

Guhathakurta, P ;

Hodge, PW ;

Karachentseva, VE ;

Sarajedini, A ;

Seitzer, P .

ASTRONOMY & ASTROPHYSICS, 2002, 389 (03) :812-824

[9] Local galaxy flows within 5 Mpc [J].

Karachentsev, ID ;

Makarov, DI ;

Sharina, ME ;

Dolphin, AE ;

Grebel, EK ;

Geisler, D ;

Guhathakurta, P ;

Hodge, PW ;

Karachentseva, VE ;

Sarajedini, A ;

Seitzer, P .

ASTRONOMY & ASTROPHYSICS, 2003, 398 (02) :479-491

[10] New distances to galaxies in the Centaurus A group [J].

Karachentsev, ID ;

Sharina, ME ;

Dolphin, AE ;

Grebel, EK ;

Geisler, D ;

Guhathakurta, P ;

Hodge, PW ;

Karachentseva, VE ;

Sarajedini, A ;

Seitzer, P .

ASTRONOMY & ASTROPHYSICS, 2002, 385 (01) :21-31

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