Details on Acronym: [WM90] | |
[WM90] | (Wilson+Mauersberger, 1990) |
Write: | <<[WM90] W 75 CO NN>> <<[WM90] W 75 CS NN>> <<[WM90] W 75 NH3 N>> |
N: | 13 |
Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
Stat: | is completely incorporated in Simbad |
Note: | Table 1: N=13 sources, among which 12 are observed in 'CO' (Nos CO 1 to CO 9, CO 11 to CO 13), 1 is observed in 'CS' (No. CS 10), and 5 in 'NH3' (Nos NH3 1 to NH3 5), with cross-id. between the differents observations |
in source: | W 75 |
Ref: | =1990A&A...239..305W |
by | WILSON T.L. , MAUERSBERGER R. |
Astron. Astrophys., 239, 305-318 (1990) | |
The internal structure of molecular clouds. I. C1C180 , C34S and NH3 maps of the DR 21/W 75S region. | |
o | Table 1: <[WM90] W 75 CO NN> (Nos 1-9, 11-13), <[WM90] W 75 CS NN> (No. 10), <[WM90] W 75 NH3 N> (Nos 1-5) |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |