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The Large‐Scale J = 3 → 2 and J = 2 → 1 CO Emission from M17 and Its Implications for Extragalactic CO Observations

  • Authors: Christine D. Wilson, John E. Howe, and Michael L. Balogh

Wilson, Howe, & Balogh 1999 The Astrophysical Journal 517 174.

  • Provider: AAS Journals

Caption: Fig. 2.

12CO/13CO ﹩J=3\rightarrow 2﹩ integrated intensity ratio for cuts at three different declinations through M17. The ratio was measured in a 15﹩\arcsec﹩ beam. The solid line connects measurements made at 0﹩\arcmin﹩ declination offset, the dashed line connects measurements made at −8﹩\arcmin﹩ declination offset, and the dotted line connects measurements made at 8﹩\arcmin﹩ declination offset. The error bars indicate a 15% calibration uncertainty. The (0, 0) position corresponds to ﹩\alpha ( 1950) =1﹩8h17m21﹩\fs﹩0, ﹩\delta ( 1950) =-1﹩6°06﹩\arcmin﹩45﹩\arcsec﹩.

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