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- W1992620906 endingPage "590" @default.
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- W1992620906 abstract "As part of an optical spectroscopic survey of nearby bright galaxies, we have identified a sample of over 200 emission-line nuclei having optical spectra resembling those of giant extragalactic H II regions. Such H II nuclei, powered by young, massive stars, are found in a substantial fraction of nearby galaxies, especially those of late Hubble type. This paper summarizes the observational characteristics of H II nuclei, considers the variation of their properties with Hubble type, and compares the nuclear H II regions with those found in galaxy disks. Similarities and differences between H II nuclei and luminous starburst nuclei are additionally noted." @default.
- W1992620906 created "2016-06-24" @default.
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- W1992620906 date "1997-10-01" @default.
- W1992620906 modified "2023-09-29" @default.
- W1992620906 title "Properties of H<scp>ii</scp>Regions in the Centers of Nearby Galaxies" @default.
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- W1992620906 doi "https://doi.org/10.1086/304642" @default.
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