Herschel-ATLAS : The surprising diversity of dust-selected galaxies in the local submillimetre Universe
MetadataShow full item record
We present the properties of the first 250 μm blind sample of nearby galaxies (15 <D <46 Mpc) containing 42 objects from the Herschel Astrophysical Terahertz Large Area Survey. Herschel's sensitivity probes the faint end of the dust luminosity function for the first time, spanning a range of stellar mass (7.4 <M* <11.3 log10 M⊙), star formation activity (-11.8 <SSFR <-8.9 log10 yr-1), gas fraction (3-96 per cent), and colour (0.6 <FUV-KS <7.0 mag). The median cold dust temperature is 14.6 K, colder than in the Herschel Reference Survey (18.5 K) and Planck Early Release Compact Source Catalogue (17.7 K). The mean dust-to-stellar mass ratio in our sample is higher than these surveys by factors of 3.7 and 1.8, with a dust mass volume density of (3.7 ± 0.7) × 105M⊙ Mpc-3. Counter-intuitively, we find that the more dust rich a galaxy, the lower its UV attenuation. Over half of our dust-selected sample are very blue in FUV-KS colour, with irregular and/or highly flocculent morphology; these galaxies account for only 6 per cent of the sample's stellar mass but contain over 35 per cent of the dust mass. They are the most actively star-forming galaxies in the sample, with the highest gas fractions and lowest UV attenuation. They also appear to be in an early stage of converting their gas into stars, providing valuable insights into the chemical evolution of young galaxies.
Clark , C J R , Dunne , L , Gomez , H L , Maddox , S , De Vis , P , Smith , M W L , Eales , S A , Baes , M , Bendo , G J , Bourne , N , Driver , S P , Dye , S , Furlanetto , C , Grootes , M W , Ivison , R J , Schofield , S P , Robotham , A S G , Rowlands , K E , Valiante , E , Vlahakis , C , van der Werf , P , Wright , A H & De zotti , G 2015 , ' Herschel-ATLAS : The surprising diversity of dust-selected galaxies in the local submillimetre Universe ' Monthly Notices of the Royal Astronomical Society , vol. 452 , no. 1 , pp. 397-430 . DOI: 10.1093/mnras/stv1276
Monthly Notices of the Royal Astronomical Society
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
DescriptionCJRC acknowledges support from the Science and Technology Facilities Council (STFC) Doctoral Training Grant scheme and the European Research Council (ERC) FP7 project DustPedia (PI J Davies). HLG and SAE acknowledge support from the STFC Consolidated Grant scheme. LD, SJM, and RJI acknowledge support from the ERC in the form of the Advanced Investigator Program, COSMICISM. KR acknowledges support from the ERC Starting Grant SEDmorph (PI V Wild).
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Showing items related by title, author, creator and subject.
Mendez Abreu, Jairo; Debattista, V. P.; Corsini, E. M.; Aguerri, J. A. L. (2014-12) - Journal articleContext. Historically, galaxy bulges were thought to be single-component objects at the center of galaxies. However, this picture is now questioned since different bulge types with different formation paths, namely classical ...
Galaxy And Mass Assembly (GAMA) : the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorph Vulcani, Benedetta; Bamford, Steven P.; Haeussler, Boris; Vika, Marina; Rojas, Alex; Agius, Nicola K.; Baldry, Ivan; Bauer, Amanda E.; Brown, Michael J. I.; Driver, Simon; Graham, Alister W.; Kelvin, Lee S.; Liske, Jochen; Loveday, Jon; Popescu, Cristina C.; Robotham, Aaron S. G.; Tuffs, Richard J. (2014-06) - Journal articleWe investigate the relationship between colour and structure within galaxies using a large, volume-limited sample of bright, low-redshift galaxies with optical-near-infrared imaging from the Galaxy And Mass Assembly survey. ...
Robotham, A. S. G.; Driver, S. P.; Davies, L. J. M.; Hopkins, A. M.; Baldry, I. K.; Agius, N. K.; Bauer, A. E.; Bland-Hawthorn, J.; Brough, S.; Brown, M. J. I.; Cluver, M.; De Propris, R.; Drinkwater, M. J.; Holwerda, B. W.; Kelvin, L. S.; Lara-Lopez, M. A.; Liske, J.; Lopez-Sanchez, A. R.; Loveday, J.; Mahajan, S.; McNaught-Roberts, T.; Moffett, A.; Norberg, P.; Obreschkow, D.; Owers, M. S.; Penny, S. J.; Pimbblet, K.; Prescott, M.; Taylor, E. N.; van Kampen, E.; Wilkins, S. M. (2014-11-11) - Journal articleWe use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift sample to fully describe the stellar mass dependence of close pairs and mergers between 10(8) and 10(12)M(circle dot). Using the analytic ...