Optically Thick Giant H II Regions with Decreasing Density Gradients in three Barred Galaxies

Details Optically Thick Giant H II Regions with Decreasing Density Gradients in three Barred Galaxies Optically Thick Giant H II Regions with Decreasing Density Gradients in three Barred Galaxies

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..256d&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Galaxies: Abundances, H Ii Regions

Scientific paper

Franco, García-Barreto, & de la Fuente (2000, hereinafter FGF00) have re-analyzed the radio continuum emission at 2, 6 and 20 cm from the circumnuclear regions of the barred galaxies NGC 1022, 1326 and 4314. The angular resolution of the observations is approximately 3.7 arcsec , roughly equiva-lent to 200 parsecs. Here we summarize the results discussed in FGF00

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