Details on Acronym: [TGC97] | |
| [TGC97] | (Tieftrunk+Gaume+Claussen+, 1997) |
| Write: | <<[TGC97] W3AaN>> |
| N: | 8+1 |
| Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | Hypercompact radio continuum sources in W 3M and W 3C observed with the VLA. Sources in W 3M form a cluster and are designated W3Ma to W3Mg, source W3d is double (d1 and d2). In W 3C, N=1 source W3Ca. These sources are also labeled following [WBN72] as [WBN72] W 3 IRS 5aN or [WBN72] W 3 IRS 4a, as W 3M is coincident with IRS 5 and W3C with IRS 4. |
| in source: | W 3 |
| Ref: | =1997A&A...318..931T |
| by | TIEFTRUNK A.R. , GAUME R.A., CLAUSSEN M.J., WILSON T.L., JOHNSTON K.J. |
| Astron. Astrophys., 318, 931-946 (1997) | |
| The H II/molecular cloud complex W3 revisited: imaging the radio continuum sources using multi-configuration, multi-frequency observations with the VLA. | |
| o | Table 3: <[TGC97] W3AaN> (Nos 3Ma-3Mc, 3Md1-3Md2, 3Me-3Mg, 3Ca) = <[WBN72] W 3 IRS NaN> (Nos 5a-5c, 5d1-5d2, 5e-5g, 4a) among which (Nos 5g, 4a) added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |