Abundance gradients in NGC 6052

Details Abundance gradients in NGC 6052 Abundance gradients in NGC 6052

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40050h&link_type=abstract

Spitzer Proposal ID #40050

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Scientific paper

There are hints in IRS low resolution data of NGC 6052 (Whelan et al. 2007) of the presence of a metallicity gradient. We propose here to investigate this in more detail by observing this galaxy for 5 hours using the SH module in mapping mode. If confirmed, this gradient would be the first one detected inside a dwarf star forming system other than the LMC.

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