Burst of star formation in detached extragalactic H II regions - A qualitative analysis

Details Burst of star formation in detached extragalactic H II regions - A qualitative analysis Burst of star formation in detached extragalactic H II regions - A qualitative analysis

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..90..385d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 90, no. 2, Feb. 1983, p. 385-389. Research supported by the Financiadora d

Astronomy and Astrophysics

Astrophysics

4

H Beta Line, H Ii Regions, Spectral Line Width, Star Formation, Calibrating, Ionized Gases, Temporal Distribution

Scientific paper

Detached extragalactic H II regions are calibrated by means of a method previously developed by Dottori (1981) for the case of the evolution of the equivalent width of the emission line H-beta with age in H II regions. The frequency distribution of ages appears to indicate that some of the regions in question have experienced other bursts of star formation that are as important as that most recently observed.

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