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• W3100612371 endingPage "162" @default.
• W3100612371 startingPage "162" @default.
• W3100612371 abstract "We present a stellar population study of three HII galaxies (Mrk 36, UM 408, and UM 461) based on the analysis of new ground-based high resolution near-infrared J, H and Kp broad-band and Br narrow-band images obtained with Gemini/NIRI. We identify and determine relative ages and masses of the elementary star clusters and/or star cluster complexes of the starburst regions in each of these galaxies by comparing the colors with evolutionary synthesis models that include the contribution of stellar continuum, nebular continuum and emission lines. We found that the current star cluster formation efficiency in our sample of low luminosity HII galaxies is ~10%. Therefore, most of the recent star formation is not in massive clusters. Our findings seem to indicate that the star formation mode in our sample of galaxies is clumpy, and that these complexes are formed by a few massive star clusters with masses > 10^4 Mo. The age distribution of these star cluster complexes shows that the current burst started recently and likely simultaneously over short time scales in their host galaxies, triggered by some internal mechanism. Finally, the fraction of the total cluster mass with respect to the low surface brightness (or host galaxy) mass, considering our complete range in ages, is less than 1%." @default.
• W3100612371 created "2020-11-23" @default.
• W3100612371 creator A5026246966 @default.
• W3100612371 creator A5055677542 @default.
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• W3100612371 date "2011-10-13" @default.
• W3100612371 modified "2023-10-18" @default.
• W3100612371 title "STAR CLUSTER COMPLEXES AND THE HOST GALAXY IN THREE H II GALAXIES: Mrk 36, UM 408, AND UM 461" @default.
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• W3100612371 doi "https://doi.org/10.1088/0004-6256/142/5/162" @default.
• W3100612371 hasPublicationYear "2011" @default.
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