Year: 2007
Type: preprint
Abstract: We present initial results from the M33 Metallicity Project. Out of the thousands of cataloged HII regions in M33, only ~30 have electron-temperature based abundances in the literature. We have obtained Keck spectroscopy of a sample of ~200 HII regions in M33, with 61 detections of the [O III] 4363 A line that can be used for determining electron temperatures, including measurements at small galactocentric radii where auroral lines are generally difficult to detect. We find an oxygen abundance gradient of -0.027 +/- 0.012 dex/kpc, in agreement with infrared measurements of the neon abundance gradient but much shallower than most previous oxygen gradient measurements. There is substantial intrinsic scatter of 0.11 dex in the metallicity at any given radius in M33, which imposes a fundamental limit on the accuracy of gradient measurements that rely on small samples of objects. Finally, we present a two-dimensional map of oxygen abundances across the southern half of M33 and discuss the evidence for deviations from axisymmetry.
Source: arXiv (Cornell University)
Authors: Simon, Joshua D., Rosolowsky, Erik
Institution: California Institute of Technology
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2089787772