Image Details

Choose export citation format:

SOFIA FIFI-LS Observations of Sgr B1: Ionization Structure and Sources of Excitation

  • Authors: Janet P. Simpson, Sean W. J. Colgan, Angela S. Cotera, Michael J. Kaufman, and Susan R. Stolovy

2018 The Astrophysical Journal Letters 867 L13.

  • Provider: AAS Journals

Caption: Figure 1.

Observed [O III] line intensities in Sgr B1. All but the darkest blue pixels have S/N > 3. The black contours are the 8.4 GHz Very Large Array (VLA) intensities from M92 and the cyan contours are the 70 μm Herschel Hi-GAL intensities (Molinari et al. 2011, 2016). (a) The [O III] 52 μm line (maximum intensity = 1.92 × 10−16 W m−2 arcsec−2). (b) The [O III] 88 μm line (maximum intensity = 1.57 × 10−16 W m−2 arcsec−2).

Other Images in This Article
Copyright and Terms & Conditions