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Massive pre-main-sequence stars in M17

Published online by Cambridge University Press:  28 July 2017

M. C. Ramírez-Tannus
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
L. Kaper
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
A. de Koter
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
F. Tramper
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
H. Sana
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
O. H. Ramírez-Agudelo
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
A. Bik
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
L. E. Ellerbroek
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
B. B. Ochsendorf
Affiliation:
API, University of Amsterdam, The Netherlands; email: m.c.ramireztannus@uva.nl
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We obtained VLT/X-shooter spectra of twelve candidate young massive stars previously selected by Hanson et al. (1997) in the giant Hii region M17. An analysis of their spectra using FASTWIND models (Puls et al. 2005) shows that they span a mass range of 6 - 20 M. We identify the presence of gaseous and dusty disks around six sources based on emission lines in the spectrum and infrared continuum excess.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

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Hosokawa, T. & Omukai, K., 2009, ApJ, 691, 823 Google Scholar
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Sana, H., Ramirez-Tannus, M., de Koter, A., & Kaper, L., et al. 2017, ArXiv:1702.02153Google Scholar