The build-up of the colour-magnitude relation

Masayuki Tanaka; Tadayuki Kodama

doi:10.1017/S1743921306005734

The build-up of the colour-magnitude relation

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

Abstract

We discuss the build-up of the colour-magnitude relation. The colour-magnitude relation first appears at the bright end and the faint end appears later. Interestingly, the build-up of colour-magnitude relation is delayed in low density environments. We suggest that galaxies follow the environment-dependent down-sizing evolution.

Original language	English
Pages (from-to)	141
Number of pages	1
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	S235
DOIs	https://doi.org/10.1017/S1743921306005734
Publication status	Published - 2006 Aug
Externally published	Yes

Keywords

Galaxies: clusters: general
Galaxies: evolution
Galaxies: fundamental parameters

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

Access to Document

10.1017/S1743921306005734

Cite this

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title = "The build-up of the colour-magnitude relation",

abstract = "We discuss the build-up of the colour-magnitude relation. The colour-magnitude relation first appears at the bright end and the faint end appears later. Interestingly, the build-up of colour-magnitude relation is delayed in low density environments. We suggest that galaxies follow the environment-dependent down-sizing evolution.",

keywords = "Galaxies: clusters: general, Galaxies: evolution, Galaxies: fundamental parameters",

author = "Masayuki Tanaka and Tadayuki Kodama",

year = "2006",

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doi = "10.1017/S1743921306005734",

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AB - We discuss the build-up of the colour-magnitude relation. The colour-magnitude relation first appears at the bright end and the faint end appears later. Interestingly, the build-up of colour-magnitude relation is delayed in low density environments. We suggest that galaxies follow the environment-dependent down-sizing evolution.

KW - Galaxies: clusters: general

KW - Galaxies: evolution

KW - Galaxies: fundamental parameters

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JO - Proceedings of the International Astronomical Union

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SN - 1743-9213

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The build-up of the colour-magnitude relation

Abstract

Keywords

ASJC Scopus subject areas

UN SDGs

Access to Document

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