High mass Star formation in the giant molecular cloud NGC 6334: an infrared view

Bibcode
2005IAUS..227..291P
DOI
10.1017/S1743921305004655
Persi, P.; Tapia, M.; Roth, M.; Gómez, M.; Marenzi, A. R.
Referencia bibliográfica

Massive star birth: A crossroads of Astrophysics, IAU Symposium Proceedings of the international Astronomical Union 227, Held 16-20 May, Italy, edited by Cesaroni, R.; Felli, M.; Churchwell, E.; Walmsley, M. Cambridge: Cambridge University Press, 2005., pp.291-296

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0
2005
Número de autores
5
Número de autores del IAC
0
Número de citas
8
Número de citas referidas
4
Descripción
Sub-Arcsec images in the JHK_s, H_2 and Br_γ of three areas (I(N), F and NGC 6334 IV (MM3)) of the giant molecular cloud NGC 6334 are presented. The preliminary results indicate the presence of a deeply embedded young stellar cluster in the northermost part of the cloud (I(N)). We have identified the exciting source of the cometary UCHII NGC 6334 F. This source has an infrared luminosity L_{IRacute;{=} 3 10^3 L_{&sun;} and a very steep infrared spectral index. Finally, a new center of massive star formation associated with the millimeter peak MM3 has been found east of the bipolar HII region NGC 6334 a.
Tipo
Sin árbitro

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