Observational and Theoretical Constraints on Singular Dark Matter Halos

Ricardo A. Flores; Joel R. Primack

doi:10.1086/187350

Observational and Theoretical Constraints on Singular Dark Matter Halos

University of Missouri-St. Louis

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	The Astrophysical Journal
Volume	427
DOIs	https://doi.org/10.1086/187350
State	Published - Jan 5 1994

Disciplines

Physics
Astrophysics and Astronomy

Access to Document

10.1086/187350License: Unspecified

Cite this

@article{75dd9a24411d446a81563cd55c16ebf1,

title = "Observational and Theoretical Constraints on Singular Dark Matter Halos",

author = "Flores, {Ricardo A.} and Primack, {Joel R.}",

note = "Abstract: The distribution of dark matter around galactic or cluster halos has usually been assumed to be approximately isothermal with a non-zero core radius, which is expected to be of the order of the size of the visible matter distribution.",

year = "1994",

month = jan,

day = "5",

doi = "10.1086/187350",

language = "American English",

volume = "427",

journal = "The Astrophysical Journal",

}

TY - JOUR

T1 - Observational and Theoretical Constraints on Singular Dark Matter Halos

AU - Flores, Ricardo A.

AU - Primack, Joel R.

N1 - Abstract: The distribution of dark matter around galactic or cluster halos has usually been assumed to be approximately isothermal with a non-zero core radius, which is expected to be of the order of the size of the visible matter distribution.

PY - 1994/1/5

Y1 - 1994/1/5

UR - https://arxiv.org/abs/astro-ph/9402004

U2 - 10.1086/187350

DO - 10.1086/187350

M3 - Article

VL - 427

JO - The Astrophysical Journal

JF - The Astrophysical Journal

ER -

Observational and Theoretical Constraints on Singular Dark Matter Halos

Disciplines

Access to Document

Other files and links

Cite this