| uthors use minus letters: W 51dN and W 51eN | |
| o | <W 51D1>, <W 51D2>, <W 51E3>, <W 51E4>, <W 51E5> |
| Auth.: | GAUME R.A.+ |
| Ref: | =1994ApJS...91..713M |
| by | MEHRINGER D.M. |
| Astrophys. J., Suppl. Ser., 91, 713-748 (1994) | |
| Radio continuum and radio recombination line observations of W 51. | |
| o | Table 2: <[M94] LL.l-B.bb> N=9, and <[M94] LL.l-B.b aN> N=22. <[M94] 49.5-0.4 aN> = W 51AN (Nos W 51E6, W 51E7, W 51I) are new |
| Ref: | =1997ApJ...488..241Z |
| by | ZHANG Q. , HO P.T.P. |
| Astrophys. J., 488, 241-257 (1997) | |
| Dynamical collapse in W51 massive cores: NH_{3} observations. | |
| o | W 51e8 = W 51E8 |
| o | <W 51E8> |
| Ref: | =2016A&A...595A..27G |
| by | GINSBURG A. , GOSS W.M., GODDI C., GALVAN-MADRID R., DALE J.E., BALLY J., BATTERSBY C.D., YOUNGBLOOD A., SANKRIT R., SMITH R., DARLING J., KRUIJSSEN J.M.D., LIU H.B. |
| Astron. Astrophys., 595A, 27-27 (2016) | |
| Toward gas exhaustion in the W51 high-mass protoclusters. | |
| o | Fig. 2, Table 3: <W 51aNN> (Nos W 51d3-d7, W 51e9-e23) added. Figs 2+A.2, Tables 3-8: <[GGG2016] arc> N=1, <[GGG2016] W51aNNw> (Nos W51d3, W51d4e-W51d4w, W51d5-W51d7, W51e8n-W51e8s, W51e9-23), <[GGG2016] W51aNNd> (Nos W51d3d, W51e11d, W51e18d), <[GGG2016] W51aNNmol> (Nos W51e8mol, W51e10mol). |
| =E= | Catalogue in electronic form as VIII/64 |
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