The SAMI galaxy survey:The discovery of a luminous, low-metallicity HII complex in the dwarf galaxy GAMA J141103.98-003242.3

We present the discovery of a luminous unresolved HII 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 o...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society
Main Authors: Richards, S. N., Schaefer, A. L., López-Sánchez, A. R., Croom, S. M., Bryant, J. J., Sweet, S. M., Konstantopoulos, I. S., Allen, J. T., Bland-Hawthorn, J., Bloom, J. V., Brough, S., Fogarty, L. M.R., Goodwin, M., Green, A. W., Ho, I. T., Kewley, L. J., Koribalski, B. S., Lawrence, J. S., Owers, M. S., Sadler, E. M., Sharp, R.
Format: Article in Journal/Newspaper
Language:English
Published: 2014
Subjects:
sami
Online Access:https://researchers.mq.edu.au/en/publications/853a4c63-8dbc-429f-add6-e9144f53f472
https://doi.org/10.1093/mnras/stu1820
http://www.scopus.com/inward/record.url?scp=84940363763&partnerID=8YFLogxK
Description
Summary:We present the discovery of a luminous unresolved HII 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 HII emission that contributes ~70 per cent of the galaxy's Hα luminosity, located at the top end of established HII region luminosity functions. For the HII complex, we measure a star formation rate of 0.147 ± 0.041 M⊙ yr -1 and a metallicity of 12+log(O/H) = 8.01 ± 0.05 that is lower than the rest of the galaxy by ~0.2 dex. Data from the HI 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 HII complex, where the kinematics of the ionized gas are well described by a rotating disc and do not show any features indicative of interactions. We showthat 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.

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