Fig. 3
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Observed ARO 12 m spectra toward IRAS 16293E shown in black and Gaussian fits as red curves. Spectra without Gaussian fits were considered nondetections, and upper limits were derived. The vertical red lines are centered at vlsr of 3.8 km/s, and the gray horizontal lines show the 1 σ noise (RMS) level. From top left to bottom right: 13CH3OH spectra offset by 50 mK, CH2DOH spectra offset by 100 mK, CHD2OH spectra offset by 50 mK, CH3CHO spectra offset by 100 mK, CH2CHCN spectra (nondetections) offset by 50mK, HCOOCH3 spectra offset by 25mK, and a single CH3OCH3 spectrum (nondetection).
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