Combining 1D image profile fitting along the outflow axis with SED fitting constrains the viewing angle of Cepheus A to about 34 degrees, but does not improve constraints for the poorly resolved G35.20-0.74N.
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Image Profile (IMPRO) Fitting of Massive Protostars. I. Method Development and Test Cases of Cepheus A and G35.20-0.74N
Combining 1D image profile fitting along the outflow axis with SED fitting constrains the viewing angle of Cepheus A to about 34 degrees, but does not improve constraints for the poorly resolved G35.20-0.74N.