University of Hertfordshire

From the same journal

By the same authors

High-resolution mass models of dwarf galaxies from LITTLE THINGS

Research output: Contribution to journalArticlepeer-review

Documents

  • 1502.01281

    Accepted author manuscript, 9.07 MB, PDF document

  • Se-Heon Oh
  • Deidre A. Hunter
  • E. Brinks
  • Bruce G. Elmegreen
  • Andreas Schruba
  • Fabian Walter
  • Michael P. Rupen
  • Lisa M. Young
  • Caroline E. Simpson
  • Megan Johnson
  • Kimberly A. Herrmann
  • Dana Ficut-Vicas
  • Phil Cigan
  • V. Heesen
  • Trisha Ashley
  • Hong-Xin Zhang
View graph of relations
Original languageEnglish
Article number180
Number of pages96
JournalThe Astronomical Journal
Volume149
Issue6
Early online date12 May 2015
DOIs
Publication statusPublished - Jun 2015

Abstract

We present high-resolution rotation curves and mass models of 26 dwarf galaxies from LITTLE THINGS. LITTLE THINGS is a high-resolution Very Large Array HI survey for nearby dwarf galaxies in the local volume within 11 Mpc. The rotation curves of the sample galaxies derived in a homogeneous and consistent manner are combined with Spitzer archival 3.6 micron and ancillary optical U, B, and V images to construct mass models of the galaxies. We decompose the rotation curves in terms of the dynamical contributions by baryons and dark matter halos, and compare the latter with those of dwarf galaxies from THINGS as well as Lambda CDM SPH simulations in which the effect of baryonic feedback processes is included. Being generally consistent with THINGS and simulated dwarf galaxies, most of the LITTLE THINGS sample galaxies show a linear increase of the rotation curve in their inner regions, which gives shallower logarithmic inner slopes alpha of their dark matter density profiles. The mean value of the slopes of the 26 LITTLE THINGS dwarf galaxies is alpha =-0.32 +/- 0.24 which is in accordance with the previous results found for low surface brightness galaxies (alpha = -0.2 +/- 0.2) as well as the seven THINGS dwarf galaxies (alpha =-0.29 +/- 0.07). However, this significantly deviates from the cusp-like dark matter distribution predicted by dark-matter-only Lambda CDM simulations. Instead our results are more in line with the shallower slopes found in the Lambda CDM SPH simulations of dwarf galaxies in which the effect of baryonic feedback processes is included. In addition, we discuss the central dark matter distribution of DDO 210 whose stellar mass is relatively low in our sample to examine the scenario of inefficient supernova feedback in low mass dwarf galaxies predicted from recent Lambda SPH simulations of dwarf galaxies where central cusps still remain.

Projects

ID: 8243530