Near-Infrared Observations of NGC 6611 {M16}

Details Near-Infrared Observations of NGC 6611 {M16} Near-Infrared Observations of NGC 6611 {M16}

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7216s&link_type=abstract

HST Proposal ID #7216

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Hst Proposal Id #7216 Young Stars And Circumstellar Material

Scientific paper

NGC 6611 has been studied in the near infrared by Hillenbrand, et al. {1993, AJ 106 1906} down to K 14.5 {3 solar masses}. This only touches the upper end of YSO population, because the field is confusion-limited from the ground. NICMOS should be able to extend the IMF statistics well into the subsolar-mass range and examine many of the EGGs {evaporating gas globules} seen in WFPC2 images. Three colors in each of the three camera fields provide color and reddening for the IMF study. Narrow band filters isolate Paschen-alpha and H_2 emission.

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