Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population

Smriti Mahajan, Michael J. Drinkwater, S. Driver, Lee S. Kelvin, A. M. Hopkins, I. Baldry, S. Phillipps, J. Bland-Hawthorn, S. Brough, J. Loveday, Samantha J. Penny, A. S. G. Robotham

Research output: Contribution to journalArticle (Academic Journal)peer-review

12 Citations (Scopus)


In this paper we aim to (i) test the number of statistically distinct classes required to classify the local galaxy population, and, (ii) identify the differences in the physical and star formation properties of visually-distinct galaxies. To accomplish this, we analyse the structural parameters (effective radius r_e, effective surface brightness within r_e (mu_e), central surface brightness (mu_0), and S'ersic index (n)), obtained by fitting the light profile of 432 galaxies (0.002z
Original languageUndefined/Unknown
Pages (from-to)2967-2984
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Publication statusPublished - 25 Sep 2014

Bibliographical note

Accepted for publication in MNRAS main journal. 17 Pages, 15 figures


  • astro-ph.GA

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