Details on Acronym: MC | |
MC | (Molecular Cloud) |
***** | Avoid the usage of MC, prefer [W95b] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [W91c] | |
[W91c] | (Wilson, 1991) |
Note: | The 3 MCld: [W91c] 1 to 3, are included in [W95b]. |
***** | Avoid the usage of [W91c], prefer [W95b] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [W95b] | |
[W95b] | (Wilson, 1995)= (MC) |
Write: | <<[W95b] MC N>> |
N: | 9 |
Object: | MCld (SIMBAD class: MolCld = Molecular Cloud) |
Stat: | is completely incorporated in Simbad |
Note: | The 3 MCld found in 1991ApJ...366L..11W, are included in [W95b]. [W91c] is superseded by [W95b]. |
in source: | IC 10 |
Ref: | =1995ApJ...448L..97W |
by | WILSON C.D. |
Astrophys. J., 448, 97-100 (1995) | |
The metallicity dependence of the CO-to-H2 conversion factor from observations of Local Group galaxies. | |
o | Table 1: <[W95b] MC N> (Nos 1-9), supersedes [W91c] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |