A multi-wavelength view of the Galactic center dust ridge reveals little star formation

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Table 2

Temperatures and masses of sub-condensations in the dust ridge in the nomenclature of Lis et al. (1999).

Position^a	T_Dust [K]	F_{870 μm,Int.} [Jy]	M_Cloud [10³M_⊙]	D_Cloud [″]

a^b	18	310	141	207
b	22	39	13	96
c	20	46	18	96
d	17	145	72	171
e	17	307	153	220
f	15	118	72	133

Notes.

^(a)

see also Fig. 2.

^(b)

M0.25+0.012.

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