Open AccessCircumstellar discs around solar mass stars in NGC 6611
Author(s) -
Oliveira J. M.,
Jeffries R. D.,
Van Loon J. Th.,
Littlefair S. P.,
Naylor T.
Publication year - 2005
Publication title -
monthly notices of the royal astronomical society: letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.067
H-Index - 122
eISSN - 1745-3933
pISSN - 1745-3925
DOI - 10.1111/j.1745-3933.2005.00020.x
Subject(s) - physics , astrophysics , stars , main sequence , orion nebula , astronomy , solar mass , star cluster
ABSTRACT We have performed IZJHKL ′ observations in NGC 6611, the young cluster that ionizes the Eagle Nebula. We have discovered a rich pre‐main sequence concentrated around the O‐stars in the cluster. As measured by their L ′‐band excesses, at least 58 ± 5 per cent of the pre‐main sequence objects (0.45 < M < 2 M ⊙ ) have circumstellar discs. By comparing this disc frequency with frequencies determined for regions where the pre‐main sequence stars are subject to less ionizing radiation, we find no evidence that the harsher environment of NGC 6611 (approximately an order of magnitude more ionizing Lyman continuum radiation than the Trapezium cluster) significantly hastens the dissipation of circumstellar discs around solar mass stars.