The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
Stott, J.P.; Sobral, D.; Smail, I.; Bower, R.; Best, P.N.; Geach, J.E.
Professor Ian Smail email@example.com
We use the HiZELS narrow-band Hα survey in combination with CANDELS, UKIDSS and WIRDS near-infrared imaging, to investigate the morphologies, merger rates and sizes of a sample of Hα emitting galaxies in the redshift range z = 0.40-2.23, an epoch encompassing the rise to the peak of the star formation rate density. Merger rates are estimated from space- and ground-based imaging using the M20 coefficient. To account for the increase in the specific star formation rate (sSFR) of the star forming `main sequence' with redshift, we normalize the star formation rates of galaxies at each epoch to the typical value derived from the Hα luminosity function. Once this trend in sSFR is removed we see no evidence for an increase in the number density of star-forming galaxies or the merger rate with redshift. We thus conclude that neither is the main driver of the enhanced star-formation rate density at z ˜ 1-2, with secular processes such as instabilities within efficiently fuelled, gas-rich discs or multiple minor mergers the most likely alternatives. However, we find that ˜40-50 per cent of starburst galaxies, those with enhanced specific star formation at their epoch, are major mergers and this fraction is redshift independent. Finally, we find the surprising result that the typical size of a star-forming galaxy of a given mass does not evolve across the redshift range considered, suggesting a universal size-mass relation. Taken in combination, these results indicate a star-forming galaxy population that is statistically similar in physical size, merger rate and mass over the ˜6 Gyr covered in this study, despite the increase in typical sSFR.
Stott, J., Sobral, D., Smail, I., Bower, R., Best, P., & Geach, J. (2013). The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey. Monthly Notices of the Royal Astronomical Society, 430(2), 1158-1170. https://doi.org/10.1093/mnras/sts684
|Journal Article Type||Article|
|Publication Date||Apr 1, 2013|
|Deposit Date||Apr 5, 2013|
|Publicly Available Date||Jul 3, 2013|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publisher||Royal Astronomical Society|
|Peer Reviewed||Peer Reviewed|
|Keywords||Galaxies, Evolution, Interactions, Star formation.|
Published Journal Article
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2013 The Authors. Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved.
You might also like
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
The importance of black hole repositioning for galaxy formation simulations