Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S292(8), p. 53-53, 2012

DOI: 10.1017/s1743921313000343

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NIR integral field spectroscopy of high mass young stellar objects

Journal article published in 2012 by K. Murakawa, S. L. Lumsden, R. D. Oudmaijer, B. Davies ORCID, M. G. Hoare
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe present K-band Integral Field Spectroscopy of six high mass young stellar objects (IRAS~18151–1208, AFGL~2136, S106~IRS4, V645 Cyg, IRAS~19065+0526, and G082.5682+ 00.4040) obtained using the adaptive optics assisted NIFS instrument mounted on the Gemini North telescope. The targets are chosen from the Red MSX Source survey led by University of Leeds. The data show the spectral features of Brγ, H2, and gas phase CO emissions and absorptions with a spectral resolution of R ≈ 5500, which allow a three-dimensional spectro-astrometric analysis of the line emissions. We discuss the results of the ionized jets and winds, and rotating CO torus.

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