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19 April 2024
 
  » arxiv » 1409.4495

 Article overview


The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3
S. N. Richards ; A. L. Schaefer ; A. R. Lopez-Sanchez ; S. M. Croom ; J. J. Bryant ; S. M. Sweet ; I. S. Konstantopoulos ; J. T. Allen ; J. Bland-Hawthorn ; J. V. Bloom ; S. Brough ; L. M. R. Fogarty ; M. Goodwin ; A. W. Green ; I.-T. Ho ; L. J. Kewley ; B. S. Koribalski ; J. S. Lawrence ; M. S. Owers ; E. M. Sadler ; R. Sharp ;
Date 16 Sep 2014
AbstractWe present the discovery of a luminous unresolved H II complex on the edge of dwarf galaxy GAMA J141103.98-003242.3 using data from the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. This dwarf galaxy is situated at a distance of ~100 Mpc and contains an unresolved region of H II emission that contributes ~70 per cent of the galaxy’s H_alpha luminosity, located at the top end of established H II region luminosity functions. For the H II complex, we measure a star-formation rate of 0.147pm0.041 M_solar yr^-1 and a metallicity of 12+log(O/H) = 8.01pm0.05 that is lower than the rest of the galaxy by ~0.2 dex. Data from the H I Parkes All-Sky Survey (HIPASS) indicate the likely presence of neutral hydrogen in the galaxy to potentially fuel ongoing and future star-forming events. We discuss various triggering mechanisms for the intense star-formation activity of this H II complex, where the kinematics of the ionised gas are well described by a rotating disc and do not show any features indicative of interactions. We show that SAMI is an ideal instrument to identify similar systems to GAMA J141103.98-003242.3, and the SAMI Galaxy Survey is likely to find many more of these systems to aid in the understanding of their formation and evolution.
Source arXiv, 1409.4495
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