Abstract
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
RCW 38, NGC 2316 and NGC 2547.
Original language | English |
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Pages (from-to) | 337 |
Journal | Extrasolar Planets: Today and Tomorrow, ASP Conference Proceedings |
Volume | 321 |
Publication status | Published - 1 Dec 2004 |