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Table 2

Parameters of the physical models for Sgr B2(N2-N5).

Parameters N2 N3 N4 N5
tstart = −1.0 × 106 yr

rstart (au) 4.46 (5) 9.46 (3) 3.21 (5) 3.06 (5)
nstart (cm−3) 3.00 (3) 3.00 (3) 3.00 (3) 3.00 (3)
Av-start (mag) 2.0 2.0 2.0 2.0
(K) 16.0 16.0 16.0 16.0
Tg-start (K) Tmin Tmin Tmin Tmin
Lstart (L) 0 0 0 0

t0 = 0

rcollapse (au) rstart rstart rstart rstart
ncollapse (cm−3) 2.14 (4) 2.19 (6) 1.00 (4) 1.86 (4)
Av-collapse (mag) 75.3 297 19.1 43.7
Td-collapse (K) Tmin Tmin Tmin Tmin
Tg-collapse (K) Tmin Tmin Tmin Tmin
Lcollapse (L) 0 0 0 0

tfinal

tfinal (yr) 2.10 (5) 2.06 (4) 3.07 (5) 2.25 (5)
rfinal (au) 1.38 (3) 5.70 (2) 1.32 (3) 1.42 (3)
nfinal (cm−3) 8.27 (7) 1.48 (8) 3.81 (7) 5.91 (7)
Av-final (mag) 500 500 500 500
Td-final (K) 400 400 400 400
Tg-final (K) 400 400 400 400
Lfinal (L) 2.63 (5) 4.71 (4) 3.92 (5) 2.82 (5)

Notes. Physical properties derived or assumed for each source at three different stages of the high-mass star formation process (see also Fig. 3). X (Y) means X × 10Y. (a) Td-start = 16 K is valid for the models with Tmin = 10 and 15 K. For Tmin = 20 K, Td-start = 20 K.

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