Star formation in NGC5471

Details Star formation in NGC5471 Star formation in NGC5471

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.324..337g&link_type=abstract

Astrophysics and Space Science, Volume 324, Issue 2-4, pp. 337-340

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a study of the star formation in the giant Hii region NGC5471 in the outskirts of M101. We have performed integrated photometry of the mean emission knots. Stellar population analysis with the code chorizos is compatible with the hypothesis that these regions have at least two different populations. The color-magnitude diagram of the region as derived from Hubble Space Telescope/WPFC2 stellar photometry shows that star formation has been going on for the last 70 Myr.

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