A Spitzer Space Telescope survey of massive young stellar objects in the G333.2−0.4 giant molecular cloud
Version of Record online: 9 NOV 2011
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society
Volume 419, Issue 1, pages 211–237, January 2012
How to Cite
Simpson, J. P., Cotera, A. S., Burton, M. G., Cunningham, M. R., Lo, N. and Bains, I. (2012), A Spitzer Space Telescope survey of massive young stellar objects in the G333.2−0.4 giant molecular cloud. Monthly Notices of the Royal Astronomical Society, 419: 211–237. doi: 10.1111/j.1365-2966.2011.19686.x
- Issue online: 13 DEC 2011
- Version of Record online: 9 NOV 2011
- Accepted 2011 August 23. Received 2011 August 23; in original form 2011 July 5
Figures 31–41. In this Supporting Information, we show images from the IRAC (panels a–d are IRAC bands 1–4, respectively) and MIPS (panels e–f are MIPS images at 24 and 70 μm) of each source. An example of the Supporting Information figures is shown in Fig. 2 for G333.131−0.560. In each figure, in panels (c)–(e), we overplot the locations of the IRS slits. In panel (b), the locations of any 6.7-GHz methanol masers (Caswell 2009) are marked with the white crosses. All images are shown in logarithmic scaling. For Fig. 31 of G332.800−0.595, the MIPS 24-μm image is replaced by the MSX 21-μm image because the MIPS 24-μm image is badly saturated. In Fig. 34, G333.212−0.105 is not visible in the MIPS 70-μm image (panel f), probably because of high background and low Spitzer resolution, but it is visible in all Herschel PACS and SPIRE 70–600 μm images.
|MNR_19686_sm_Figs31to41.zip||390K||Supporting info item|
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