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Infant mortality of star clusters: On the origin of the diffuse uv emission

  • Anne Pellerin
  • , Martin J. Meyer
  • , Jason Harris
  • , Daniela Calzetti

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

We present HST images in which we discovered the presence of a large number of massive stars in the field of the two galaxies NGC 1313 and NGC 4449. These massive stars, not in obvious groups or clusters, are known to produce a significant amount of UV radiation, and to live for at most 25 Myr. We think that these stars are the main source of diffuse UV emission first observed by Meurer et al. (1995) in starburst galaxies. We also propose that the infant mortality of star clusters, an early evolutionary stage of star clusters which kills 90% of them within 10 Myr, is a physical process that can explain how these young stars could end up in the field so quickly. We will also present preliminary stellar 2-points correlation functions for the two galaxies.

Original languageEnglish
Title of host publicationAstrophysics and Space Science Proceedings
EditorsMiguel Chavez Dagostino, Emanuele Bertone, Daniel Rosa Gonzalez, Lino Hector Rodriguez-Merino
PublisherSpringer Science and Business Media B.V.
Pages141-146
Number of pages6
ISBN (Electronic)9780387876214
ISBN (Print)9780387727677, 9780387876207, 9781402055720, 9781402069321, 9781402088674, 9781402091896, 9781441981608, 9781441983688, 9783540758259, 9783642033230, 9783642103216, 9783642103513, 9783642113406, 9783642172502, 9789048133994, 9789048134984
DOIs
StatePublished - 2009
EventInternational Conference on Ultraviolet Properties of Evolved Stellar Populations, 2007 - Puerto Vallarta, Mexico
Duration: Apr 16 2007Apr 20 2007

Publication series

NameAstrophysics and Space Science Proceedings
Volume0

Conference

ConferenceInternational Conference on Ultraviolet Properties of Evolved Stellar Populations, 2007
Country/TerritoryMexico
CityPuerto Vallarta
Period04/16/0704/20/07

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