Details on Acronym: [CWB94] | |
| [CWB94] | (Colbert+Wilson+Bland-Hawthorn, 1994) |
| Write: | <<[CWB94] N>> <<[CWB94] NN>> <<[CWB94] WN>> <<[CWB94] WW>> <<[CWB94] Nd>> |
| N: | 18 |
| Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
| Note: | VLA map of NGC 6240. The nuclear region is designated 'N', with 3 sources (Nos N1-N3), a diffuse nuclear region 'Nd', and a southern source 'S'. The Western Arm is designated 'W', with clumps (Nos W0-W4). Other radio components are found later: (S1, S2, E1, NW, NE, SE). |
| in source: | NGC 6240 |
| Ref: | =1994ApJ...436...89C |
| by | COLBERT E.J.M. , WILSON A.S., BLAND-HAWTHORN J. |
| Astrophys. J., 436, 89-101 (1994) | |
| The radio emission from the ultraluminous far-infrared galaxy NGC 6240. | |
| o | N1* and N2*, unresolved components of N1 and N2, not in SIMBAD. |
| o | Figs 2, 3, Table 3: <[CWB94] AN> (Nos N, N1-N3), <[CWB94] WN> (Nos S, W, W1-W4), <[CWB94] Ad> (No. Nd). |
| Ref: | =2004AJ....127..239G |
| by | GALLIMORE J.F. , BESWICK R. |
| Astron. J., 127, 239-251 (2004) | |
| Parsec-scale radio structure of the double active nucleus of NGC 6240. | |
| o | Par. 2.1: the candidate radio supernova is [G2000] J165258.8998+022403.591, later designated as [CWB94] S2. |
| o | <[CWB94] WN> (No. S1) added. |
| Ref: | =2007ApJ...659..283I |
| by | IONO D. , WILSON C.D., TAKAKUWA S., YUN M.S., PETITPAS G.R., PECK A.B., HO P.T.P., MATSUSHITA S., PIHLSTROM Y.M., WANG Z. |
| Astrophys. J., 659, 283-295 (2007) | |
| High-resolution imaging of warm and dense molecular gas in the nuclear region of the luminous infrared galaxy NGC 6240. | |
| o | 2 QSOs not identified : 1743-038 and 1549+026 |
| o | <[CWB94] WN> (No. S2) added. |
| Ref: | =2007ApJ...661..173B |
| by | BAAN W.A. , HAGIWARA Y., HOFNER P. |
| Astrophys. J., 661, 173-184 (2007) | |
| H I and OH absorption toward NGC 6240. | |
| o | Table 1: <[CWB94] WN> (Nos W0, E1) added, <[CWB94] WW> (Nos NW, NE, SE). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |