DARK MATTER AND COOLING FLOWS

被引：0

作者：

CARR, BJ ^{[1
]}

ASHMAN, KM ^{[1
]}

机构：

[1] UNIV LONDON QUEEN MARY COLL,SCH MATH SCI,LONDON E1 4NS,ENGLAND

来源：

IAU SYMPOSIA | 1988年 / 130期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：429 / 435

页数：7

共 50 条

[41] Gravitational cooling and density profile near caustics in collisionless dark matter haloes
Mohayaee, R
Shandarin, SF
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 366 (04) : 1217 - 1229
[42] Solving the cooling flow problem of galaxy clusters by dark matter neutralino annihilation
Totani, T
PHYSICAL REVIEW LETTERS, 2004, 92 (19) : 191301 - 1
[43] Solving the cooling flow problem of galaxy clusters by dark matter neutralino annihilation
Totani, T
NEW ASTRONOMY REVIEWS, 2005, 49 (2-6) : 205 - 208
[44] DARK-MATTER FROM COSMIC FLOWS - HOW MUCH - WHERE - WHAT IS IT
DEKEL, A
NUCLEAR PHYSICS B, 1995, : 425 - 434
[45] Dark sector unifications: Dark matter-phantom energy, dark matter - constant w dark energy, dark matter-dark energy-dark matter
Perkovic, Dalibor
Stefancic, Hrvoje
PHYSICS LETTERS B, 2019, 797
[46] Measuring the cold dark matter power spectrum from variations of Hubble flows
Shi, XD
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 290 (01) : L7 - L9
[47] Cooling flows
Fabian, AC
TRACING COSMIC EVOLUTION WITH GALAXY CLUSTERS, PROCEEDINGS, 2002, 268 : 177 - 186
[48] Dark matter from dark photons: A taxonomy of dark matter production
Hambye, Thomas
Tytgat, Michel H. G.
Vandecasteele, Jerome
Vanderheyden, Laurent
PHYSICAL REVIEW D, 2019, 100 (09)
[49] Interacting dark matter disguised as warm dark matter
Boehm, C
Riazuelo, A
Hansen, SH
Schaeffer, R
PHYSICAL REVIEW D, 2002, 66 (08)
[50] Dark Matter 2. Dark Matter in the Universe
Phookun, Bikram
Nath, Biman
RESONANCE-JOURNAL OF SCIENCE EDUCATION, 2005, 10 (12): : 76 - 82

← 1 2 3 4 5 →