Metallicity Gradients and Gas Flows in Galaxy Pairs

We present the first systematic investigation into the metallicity gradients in galaxy close pairs. We determine the metallicity gradients for eight galaxies in close pairs using H II region metallicities obtained with high signal-to-noise multi-slit observations with the Keck LRIS Spectrograph. We...

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Bibliographic Details
Published in:Astrophysical journal. Letters 2010-09, Vol.721 (1), p.L48-L52
Main Authors: Kewley, Lisa J, Rupke, David, Jabran Zahid, H, Geller, Margaret J, Barton, Elizabeth J
Format: Article
Language:English
Subjects:
ABUNDANCE
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
FLUID FLOW
GALAXIES
GAS FLOW
MILKY WAY
NOISE
SIGNALS
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Summary:We present the first systematic investigation into the metallicity gradients in galaxy close pairs. We determine the metallicity gradients for eight galaxies in close pairs using H II region metallicities obtained with high signal-to-noise multi-slit observations with the Keck LRIS Spectrograph. We show that the metallicity gradients in close pairs are significantly shallower than gradients in isolated spiral galaxies such as the Milky Way, M83, and M101. These observations provide the first solid evidence that metallicity gradients in interacting galaxies are systematically different from metallicity gradients in isolated spiral galaxies. Our results suggest that there is a strong relationship between metallicity gradients and the gas dynamics in galaxy interactions and mergers.
ISSN:2041-8205
2041-8213
DOI:10.1088/2041-8205/721/1/L48