What Can We Learn from Protoplanetary Disk Frequency in Young Clusters?

  • S. R. Fernandes
  • , P. S. Teixeira
  • , J. C. Correia
  • , J. F. Alves
  • , F. D. Santos
  • , E. A. Lada
  • , C. J. Lada

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The origin and evolution of circumstellar disks is one of the main scientific quests intimately related with planetary formation, since disks are known to be planetary nurseries. A study of statistically significant young stellar populations, in different evolutionary stages and astrophysical environments, can provide fundamental tests for theories of disk and planet formation. We are presently conducting a systematic broadband infrared wavelength study of ten young clusters of different ages, in order to compare their circumstellar disk frequency. We report our results of JHK photometry of three nearby clusters of our sample, RCW 38, NGC 2316 and NGC 2547.
Original languageEnglish
Title of host publicationExtrasolar Planets
Subtitle of host publicationToday and Tomorrow
EditorsJ. P. Beaulieu, A. Lecavelier des Etangs, C. Terquem
Pages237-243
Number of pages7
Volume321
ISBN (Electronic)978-1-58381-256-3
Publication statusPublished - 1 Dec 2004
EventAstronomical Society of the Pacific Conference - Institut D'Astrophysique de Paris, France
Duration: 30 Jun 20034 Jul 2003

Conference

ConferenceAstronomical Society of the Pacific Conference
Abbreviated titleASP
Country/TerritoryFrance
Period30/06/034/07/03

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