| (Not yet in Simbad) | |
| Write: | << W75N(H2O)>> << W75N(OH)>> << W75N(CO)>> << W75N(HCN)>> << W75N(IR)>> |
| N: | 3+4+5 |
| Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | Radio continuum sources in W 75N: N=3 sources (Nos A-C), named [HRB1] W75N(A) to C, [HRB1] W75N(B) been divided into 4 components [HRB1] W75N(Ba) to [HRB1] W75N(Bd). N=5 sources in H2O, OH, CO, HCN, and IR |
| in source: | W 75:W 75N = W 75N |
| Ref: | =1981ApJ...244...76H |
| by | HASCHICK A.D. , REID M.J., BURKE B.F., MORAN J.M., MILLER G. |
| Astrophys. J., 244, 76-87 (1981) | |
| VLBI aperture synthesis observations of the OH maser source W75N. | |
| o | Table 2: <[HRB81] W75N(A)> (Nos A-C), <[HRB81] W75N(H2O)>, <[HRB81] W75N(OH)>, <[HRB81] W75N(CO)>, <[HRB81] W75N(HCN)>, <[HRB81] W75N(IR)> |
| Ref: | =1994A&A...284..215H |
| by | HUNTER T.R. , TAYLOR G.B., FELLI M., TOFANI G. |
| Astron. Astrophys., 284, 215-226 (1994) | |
| Water masers embedded in ultracompact HII regions : the W 75N cloud core. | |
| o | Table 1: <[HTF94] W75N N> (Nos 1-5). Table 2, Fig.1: <[HRB81] W75N(Ba)> (Nos Ba-Bd). |
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