Details on Acronym: [WBH2013] | |
| [WBH2013] | (Wang+Bourke+Hogerheijde+, 2013) |
| Write: | <<[WBH2013] SMMN>> |
| N: | 5 |
| Object: | (Submm) (SIMBAD class: smmRad = Sub-Millimetric Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | SMA 354GHz observations of N=5 emission peak in the massive protocluster W3 IRS5. |
| in source: | NAME W 3 IRS 5 Cluster |
| Ref: | =2013A&A...558A..69W |
| by | WANG K.-S. , BOURKE T.L., HOGERHEIJDE M.R., VAN DER TAK F.F.S., BENZ A.O., MEGEATH S.T., WILSON T.L. |
| Astron. Astrophys., 558A, 69-69 (2013) | |
| Dense molecular cocoons in the massive protocluster W3 IRS 5: a test case for models of massive star formation. | |
| o | Table 1: <[WBH2013] SMMN> (Nos SMM1-SMM5). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |