High-angular resolution observations of methanol in the infrared dark cloud core G11.11-0.12P1

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Table 2

Parameters of the observed continuum emission.

Frequency	Peak Intensity Position		Peak Intensity	Flux density^a	Deconvolved angular size^b	Mass^c
(GHz)	RA (J2000)	Dec (J2000)	(mJy beam^-1)	(mJy)		(M_⊙)

96.6	18^h10^m2828	−19°22′305	7.0	20.2		37
240.3	18^h10^m2829	−19°22′305	30.8	208.6		13

Notes.

^(a)

Flux density was obtained by summing the continuum emission above 3σ level within a polygon encompassing the core.

^(b)

Major axis × minor axis, at FWHM; position angle of major axis from fits of elliptical Gaussian.

^(c)

Assuming a distance of 3.6 kpc and dust temperature of 60 K.

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