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Haro 11 | Mrk 1089 | NGC 1705 | ||||
no submm | submm | no submm | submm | no submm | submm | |
![]() ![]() |
6.2 ![]() |
1.7 ![]() ![]() ![]() |
3 ![]() |
5.12 ![]() ![]() ![]() |
2.9 ![]() |
1.3 ![]() ![]() ![]() |
![]() |
0.22 | 0.1 | 0.18 | 0.18 | 0.11 | 4.4 ![]() |
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1.88 | 1.73 | 2.21 | 2.18 | 2.5 | 1.84 |
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12.2 | 1.44 | 1.5 | 0.82 | 3.68 | 9 ![]() |
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1.3 ![]() |
5.77 ![]() |
3.84 ![]() |
3.5 ![]() |
1.47 ![]() |
8.67 ![]() |
![]() ![]() |
![]() |
2.7 ![]() |
4.1 ![]() |
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![]() ![]() |
6 ![]() |
0.17 | 10-3 | 1.9 ![]() |
7 ![]() |
3.2 ![]() |
a
Bold numbers are
the dust mass and the dust-to-gas mass ratio values of our prefered SED
for the galaxy Mrk 1089. b HI mass associated with the aperture chosen for the dust mass determination, namely 80% of the the total HI mass. |
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