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The ALMA View of the OMC1 Explosion in Orion

  • Authors: John Bally, Adam Ginsburg, Hector Arce, Josh Eisner, Allison Youngblood, Luis Zapata, and Hans Zinnecker

2017 The Astrophysical Journal 837 60.

  • Provider: AAS Journals

Caption: Figure 5.

North–south cuts across the OMC1 outflow at the R.A. of the explosion center showing the radial velocity structure over a 80″  (∼5 × 1017 cm or 0.16 pc) spatial region centered on the outflow in the 230 GHz CO J = 2−1 emission line. Three north–south strips (equivalent to “long-slit” spectra) separated by 0.″6  are shown in red, green, and blue. The green channel is centered at R.A. = 05h35m14.ˢ364. The red channel shows the “long-slit” spectrum 0.″6 to the east of this position; the blue channel shows the “long-slit” spectrum 0.″6 west of this position. The intensity scale ranges from −10 to 80 K. An animated version of Figure 5 showing the long-slit spectrum (upper panel) in which the slit orientation pivots 360° around the explosion center (lower panel) is provided in the online Journal. The animation is 15 s in duration.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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