Details on Acronym: [WWS2022] | |
[WWS2022] | (Wu+Wu+Sotnikova+, 2022) |
Write: | <<[WWS2022] AN>> <<[WWS2022] OHN>> <<[WWS2022] HI>> |
N: | 18+2+1 |
Object: | Part of G + (Rad) + Maser (SIMBAD class: Unknown = Object of Unknown Nature) |
Note: | N=18 spots, N=2 masers, and N=1 HI sources in Zw II 096. Use of European Very Long Baseline Interferometry (VLBI) Network (EVN), VLBA, VLA, and ALMA archival data. |
in source: | IRAS 20550+1656 = Zw II 96 |
Ref: | =2022A&A...661A.125W |
by | WU H. , WU Z., SOTNIKOVA Y., CHEN Y., ZHANG B., MUFAKHAROV T., SHEN Z., CHEN X., MIKHAILOV A., MINGALIEV M., HAN X.L., MISRA P. |
Astron. Astrophys., 661A, 125-125 (2022) | |
Radio properties of the OH megamaser galaxy IIZw 096. | |
o | Fig. 1, Table 2: <[WWS2022] AN> (Nos A0-A3, B0-B6, C0-C3, D0-D2), <[WWS2022] OHN> (Nos OH1-OH2), <[WWS2022] HI> N=1. Fig. A.4, Table A.3: <[WWS2022] HIN> (Nos HI1-HI7). |
Origin | of the Acronym: D = Assigned by the Dictionary of Acronyms |