Spectroscopy and abundances of SINGS galaxies (Moustakas+, 2010)

Details Spectroscopy and abundances of SINGS galaxies (Moustakas+, 2010) Spectroscopy and abundances of SINGS galaxies (Moustakas+, 2010)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21900233m&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/190/233. Originally published in: 2010ApJS..190..233M

Computer Science

Surveys, Galaxies: Ir, Spectroscopy, Equivalent Widths, Abundances, H Ii Regions

Scientific paper

The optical spectra were obtained between 2001 November and 2006 May at the Bok 2.3m telescope on Kitt Peak for galaxies in the northern hemisphere, and at the CTIO 1.5m telescope for galaxies in the southern hemisphere.
The SINGS sample (Kennicutt et al., 2003PASP..115..928K), comprising 75 galaxies, is intended to be a valuable representative set of local galaxies that are not ultraluminous, and whose moderate distances ensure that the properties of the interstellar medium can be studied at relatively small spatial scales (a few hundreds of parsecs at the shortest wavelengths).
(5 data files).

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