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  5. The causes of the red sequence, the blue cloud, the green valley, and the green mountain
 
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The causes of the red sequence, the blue cloud, the green valley, and the green mountain
File(s)
sty2220.pdf (1 MB)
Published version
Author(s)
Eales, Stephen A
Baes, Maarten
Bourne, Nathan
Bremer, Malcolm
Brown, Michael JI
more
Type
Journal Article
Abstract
The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud, with the green valley in between. We show that the galaxies found in a submillimetre survey have almost the opposite distribution in this diagram, forming a ‘green mountain’. We show that these distinctive distributions follow naturally from a single, continuous, curved Galaxy Sequence in a diagram of specific star formation rate versus stellar mass, without there being the need for a separate star-forming galaxy main sequence and region of passive galaxies. The cause of the red sequence and the blue cloud is the geometric mapping between stellar mass/specific star formation rate and absolute magnitude/colour, which distorts a continuous Galaxy Sequence in the diagram of intrinsic properties into a bimodal distribution in the diagram of observed properties. The cause of the green mountain is Malmquist bias in the submillimetre waveband, with submillimetre surveys tending to select galaxies on the curve of the Galaxy Sequence, which have the highest ratios of submillimetre-to-optical luminosity. This effect, working in reverse, causes galaxies on the curve of the Galaxy Sequence to be underrepresented in optical samples, deepening the green valley. The green valley is therefore not evidence (1) for there being two distinct populations of galaxies, (2) for galaxies in this region evolving more quickly than galaxies in the blue cloud and the red sequence, and (3) for rapid-quenching processes in the galaxy population.
Date Issued
2018-11-01
Date Acceptance
2018-08-10
Citation
Monthly Notices of the Royal Astronomical Society, 2018, 481 (1), pp.1183-1194
URI
http://hdl.handle.net/10044/1/66395
DOI
https://www.dx.doi.org/10.1093/mnras/sty2220
ISSN
0035-8711
Publisher
Oxford University Press (OUP)
Start Page
1183
End Page
1194
Journal / Book Title
Monthly Notices of the Royal Astronomical Society
Volume
481
Issue
1
Copyright Statement
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Sponsor
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council
Science and Technology Facilities Council (STFC)
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000449651400083&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Grant Number
ST/L001314/1
ST/K006401/1
ST/M003558/1
ST/P000568/1
ST/N005317/1
ST-N000838
ST/N000838/1
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
galaxies: evolution
galaxies: general
ATLAS DATA RELEASE
LATE-TYPE GALAXIES
STAR-FORMATION
HERSCHEL-ATLAS
ANGULAR-MOMENTUM
MASS
GAMA
EVOLUTION
MULTIWAVELENGTH
COUNTERPARTS
Publication Status
Published
Date Publish Online
2018-08-23
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