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Star |
![]() |
Integrated flux(b) | Intensity(b) |
![]() |
H2 mass upper limits(b, c) | |||||
HD | (![]() |
(erg s-1 cm-2) | (erg s-1 cm-2 sr-1) | (cm-2) | (
![]() |
|||||
150 K | 300 K | 1000 K | 150 K | 300 K | 1000 K | |||||
142527 | 17.0351 |
![]() |
<2.5 ![]() |
9.4 ![]() |
6.1 ![]() |
1.4 ![]() |
1.9 ![]() |
1.2 ![]() |
3.3 ![]() |
|
169142 | 17.0343 | <1.8 ![]() |
<4.2 ![]() |
1.6 ![]() |
1.0 ![]() |
2.4 ![]() |
3.5 ![]() |
2.1 ![]() |
6.1 ![]() |
|
150193A | 17.0349 | <2.1 ![]() |
<5.0 ![]() |
1.9 ![]() |
1.2 ![]() |
2.8 ![]() |
4.5 ![]() |
2.7 ![]() |
7.7 ![]() |
|
163296 | 17.0345 | <2.8 ![]() |
<6.7 ![]() |
2.5 ![]() |
1.6 ![]() |
3.8 ![]() |
3.9 ![]() |
2.4 ![]() |
6.9 ![]() |
|
100546 | 17.0363 | <1.4 ![]() |
<3.3 ![]() |
1.2 ![]() |
7.9 ![]() |
1.9 ![]() |
1.4 | 8.4 ![]() |
2.4 ![]() |
Notes. (a) expected position of the line in the observed spectra by
correcting the radial velocity of the star for the epoch of
observation. (b) 3
upper confidence limits. (c) masses of H2 are calculated assuming the distances quoted
in Table 1.
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