Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)

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Volume 559 (November 2013)

A&A, 559 (2013) A47

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201321096e]

Table 4

Properties of the continuum emission toward Sgr B2(N) and (M).

f^a	F_f^b	S_f^c	Size^d	Ω^e	T^f	S_f/ΩB_f^g
(GHz)	(Jy/beam)	(Jy)	(″×″)	(10^-10 sr)	(K)
(1)	(2)	(3)	(4)	(5)	(6)	(7)

Sgr B2(N)
85	–	0.90	3.2 × 2.8	2.1	200	0.10
					150	0.13
					100	0.20
91	2.0	–	12.2 × 4.4	14.3	200	0.03
					150	0.04
					100	0.06
227	20.0	–	4.5 × 3.7	4.4	200	0.15
					150	0.20
					100	0.30

Sgr B2(M)
85	–	4.38	4.8 × 3.2	3.6	200	0.28
					150	0.37
					100	0.56
91	3.0	–	10.5 × 4.9	13.7	200	0.04
					150	0.06
					100	0.09
153	3.5	–	6.5 × 3.0	5.2	200	0.05
					150	0.06
					100	0.10
227	12.0	–	4.5 × 3.7	4.4	200	0.09
					150	0.12
					100	0.18

Notes.

^(a)

Frequency.

^(b)

Peak flux density from de Vicente et al. (2000) at 91 GHz, Furuya et al. (2003) at 153 GHz, Lis et al. (1993) at 227 GHz.

^(c)

Flux density from Liu & Snyder (1999) at 85 GHz.

^(d)

Beam size or size of the box over which the flux density was integrated.

^(e)

Solid angle of the beam or integration box.

^(f)

Assumed temperature for the Planck function.

^(g)

Ratio of the measured continuum flux density to the product of the solid angle Ω and the Planck function B_f(T).

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