The causes of the red sequence, the blue cloud, the green valley, and the green mountain. Issue 1 (23rd August 2018)
- Record Type:
- Journal Article
- Title:
- The causes of the red sequence, the blue cloud, the green valley, and the green mountain. Issue 1 (23rd August 2018)
- Main Title:
- The causes of the red sequence, the blue cloud, the green valley, and the green mountain
- Authors:
- Eales, Stephen A
Baes, Maarten
Bourne, Nathan
Bremer, Malcolm
Brown, Michael J I
Clark, Christopher
Clements, David
de Vis, Pieter
Driver, Simon
Dunne, Loretta
Dye, Simon
Furlanetto, Cristina
Holwerda, Benne
Ivison, R J
Kelvin, L S
Lara-Lopez, Maritza
Leeuw, Lerothodi
Loveday, Jon
Maddox, Steve
Michałowski, Michał J
Phillipps, Steven
Robotham, Aaron
Smith, Dan
Smith, Matthew
Valiante, Elisabetta
van der Werf, Paul
Wright, Angus - Abstract:
- 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 thanABSTRACT: 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. … (more)
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 481:Issue 1(2018)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 481:Issue 1(2018)
- Issue Display:
- Volume 481, Issue 1 (2018)
- Year:
- 2018
- Volume:
- 481
- Issue:
- 1
- Issue Sort Value:
- 2018-0481-0001-0000
- Page Start:
- 1183
- Page End:
- 1194
- Publication Date:
- 2018-08-23
- Subjects:
- galaxies: evolution -- galaxies: general
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/sty2220 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
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British Library HMNTS - ELD Digital store - Ingest File:
- 15710.xml