Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-09-18
Astronomy and Astrophysics
Astrophysics
Sf2a 2007 PNPS
Scientific paper
The number and the nature of emission line stars in the young open cluster NGC6611 is still the object of debates. Due to the presence of a strong and variable nebulosity in the cluster, the number of emission line stars is highly depending on the technique and the resolution used for the observations. Thanks to observations with the ESO-WFI, in slitless spectroscopic mode, and with the VLT-GIRAFFE we have been able to disentangle the circumstellar and nebular emissions. We confirm the small number of true emission line objects and we precise their nature: mainly Herbig Be stars.
Baade Dietrich
Fabregat Juan
Floquet Michele
Frémat Yves
Hubert Anne-Marie
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