Hot HCN around young massive stars at 0.1′′ resolution

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Volume 529 (May 2011)

A&A, 529 (2011) A76

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Table 1

Observational summary.

Source	Pointing center		Continuum beam^a	Line beam^a	rms 1 km s^-1^b	rms continuum^b	rms integrated line^b
	RA(J2000)	Dec(J2000)	(′′;°)	(′′;°)	(mJy/Beam)	(K)	(K km s^-1)

G10.47+0.03	18 08 38.236	–19 51 50.3	0.12 × 0.06;82	0.14 × 0.1;69	2.3	45	900
SgrB2-N	17 47 19.902	–28 22 17.8	0.12 × 0.08;60	0.15 × 0.11;51	3.0	75	1300
SgrB2-M	17 47 20.202	–28 23 05.3	0.12 × 0.08;63	0.15 × 0.11;51	3.3	95	1400

Notes.

^(a)

Different weighting schemes were used for continuum and line images. Major and minor axis and position angle are given.

^(b)

rms noise in 1 km s^-1 channel, continuum and integrated line maps (Figs. 2, 4, and 6). The noise is evaluated over a box from − 2 to − 1′′ in both RA and Dec relative to the phase center.

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