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Gemini, SOFIA, and ATCA Reveal Very Young, Massive Protostars in the Collapsing Molecular Cloud BYF 73

  • Authors: Rebecca L. Pitts, Peter J. Barnes, Stuart D. Ryder, and Dan Li

2018 The Astrophysical Journal Letters 867 L7.

  • Provider: AAS Journals

Caption: Figure 3.

Flux densities of T-ReCS-detected sources in both T-ReCS and Spitzer/IRAC data. Secure detections are indicated by points connected by solid lines; 3σ upper limits are indicated by symbols connected to the other data by dotted lines. As we obtained only a partial image for MIR 3 at 18.3 μm, its flux density is at least twice the indicated lower limit. Error bars are 1σ noise values, but the calibration uncertainty is ±15% for these data after allowing for subtraction of variable background emission.

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