Core | R | ![]() |
![]() |
Peak
![]() |
![]() |
![]() |
![]() |
(pc) | (
![]() |
(
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(
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(![]() |
(![]() |
||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
00117+6412 |
0.57 | 2.58 | 4.29 | 5.13 | 1.8E+2 | 4.8E+2 | 2.7 |
00557+5612 | 1.08 | 2.05 | 1.47u | 1.66 | 6.6E+2 | 5.7E+2 | 0.9 |
03101+5821 | >1.08 | 2.52 | 1.20 | 1.76 | >5.8E+2 | 8.6E+2 | 1.5 |
03260+3111a | >0.23 | 3.05 | 0.29 | 15.96 | >1.6E+2 | 2.6E+2 | 1.6 |
03260+3111NEs | 0.11 | 2.51 | ... | 15.96 | 8.0E+1 | 8.8E+1 | 1.1 |
03414+3200 | >0.34 | 1.92 | 0.05u | 5.35 | >8.5E+1 | 1.6E+2 | 1.8 |
05168+3634 | >2.41 | 2.86 | 17.13 | 1.57 | >1.2E+4 | 2.4E+3 | 0.2 |
05168+3634SWs | 0.60m | 2.61 | ... | 1.57 | 3.0E+3 | 5.2E+2 | 0.2 |
06067+2138 | 0.55 | 3.36b | 0.03u | 3.83 c | 2.5E+2 | 7.8E+2 | 3.1 |
06103+1523 | 1.97 | 2.56 | 9.49 | 1.02 | 2.8E+3 | 1.6E+3 | 0.6 |
07024-1102 | >0.11m | 1.99 | 0.57 | 64.73c | >9.0E+0 | 5.8E+1 | 6.4 |
20067+3415 | 1.76 | 3.80b | 1.14 | 1.14 | 3.9E+3 | 3.2E+3 | 0.8 |
20067+3415NEs | 0.45m | 3.67 | ... | 1.14 | 9.7E+2 | 7.5E+2 | 0.8 |
20149+3913 | 0.43 | 3.19 | 0.30u | 2.62 | 1.4E+3 | 5.5E+2 | 0.4 |
20151+3911a | >1.30 | 3.83 | 0.70u | 2.62 | >4.1E+3 | 2.4E+3 | 0.6 |
21391+5802 | 0.32 | 2.78 | 0.26 | 11.87c | 1.3E+2 | 3.1E+2 | 2.4 |
22198+6336 | 1.22 | 2.21b | 1.53u | 2.39 | 1.7E+3 | 7.5E+2 | 0.4 |
22506+5944 | 1.31 | 2.88 | 6.83 | 1.40 | 1.0E+3 | 1.4E+3 | 1.4 |
Average![]() |
0.98 | 2.80 | 3.02 | 4.95 | 1.9E+3 | 1.1E+3 | 1.3 |
Note. a Not
guide IRAS source. Luminosity
calculated based on IRAS fluxes and distance:
03260+3111 at
0.4 kpc (Harju
et al. 1998) and 20151+3911 at 1.7 kpc
(Motte
et al. 2007). b Average
spectrum fitted with
two Gaussian profiles, list the stronger one. c No
12CO data, density calculated by assuming
reasonable
(see text). m Core's
angular diameter
comparable to beamwidth, marginally resolved. s Sourceless
core. u Upper
limit.
Average
calculating does not
include values of marginally resolved cores, except for the line width
column.
*
/
.
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