Dark matter in dumbbell galaxies.: International Conference on Dynamics and Interactions of Galaxies

S. Casertano; E. A. Valentijn

Dark matter in dumbbell galaxies. International Conference on Dynamics and Interactions of Galaxies

Astronomy

Research output: Contribution to conference › Paper › Academic

Abstract

A morphologically well-defined sample of dumbbell systems, with measured projected separations and velocity differences, provides evidence of the presence of dark matter on a scale of about 50 kpc.

Original language	English
Pages	365-366
Publication status	Published - 1988

Keywords

Galaxy Pairs: Dark Matter

Access to Document

http://adsabs.harvard.edu/abs/1990dig..book..365C

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Cite this

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title = "Dark matter in dumbbell galaxies.: International Conference on Dynamics and Interactions of Galaxies",

abstract = "A morphologically well-defined sample of dumbbell systems, with measured projected separations and velocity differences, provides evidence of the presence of dark matter on a scale of about 50 kpc.",

keywords = "Galaxy Pairs: Dark Matter",

author = "S. Casertano and Valentijn, {E. A.}",

year = "1988",

language = "English",

pages = "365--366",

}

TY - CONF

T1 - Dark matter in dumbbell galaxies.

T2 - International Conference on Dynamics and Interactions of Galaxies

AU - Casertano, S.

AU - Valentijn, E. A.

PY - 1988

Y1 - 1988

N2 - A morphologically well-defined sample of dumbbell systems, with measured projected separations and velocity differences, provides evidence of the presence of dark matter on a scale of about 50 kpc.

AB - A morphologically well-defined sample of dumbbell systems, with measured projected separations and velocity differences, provides evidence of the presence of dark matter on a scale of about 50 kpc.

KW - Galaxy Pairs: Dark Matter

M3 - Paper

SP - 365

EP - 366