Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati WAF2016] MMNa$
.

Details on Acronym:   [WAF2016]
  
[WAF2016] (Wang+Audard+Fontani+, 2016)
Write:<<[WAF2016] VLAN>>
<<[WAF2016] clump>>
<<[WAF2016] MMNa>>
<<[WAF2016] HMSC-W>>
N: 2+1+10+2
Object:(Rad) + (mm)  (SIMBAD class: Radio = Radio Source)
Stat.in SIMBAD: Fig.5 [WAF2016] HMSC-W and [WAF2016] HMSC-E not in Simbad.
Note:Centimeter and millimeter continuum observations and molecular line observations of the protocluster associated with IRAS 22134+5834.
EVLA (6.0, 3.6, 1.3, 0.7cm) observations of N=2 radio sources.
CARMA (3mm), PdBI (2mm), and SMA (1.3mm) observations of N=1 clump at 3 millimeter, N=6 millimeter continuum cores at 2mm with two being resolved at 1.3mm.
CARMA and VLA molecular line observations of N=2 high-mass starless clumps (HMSC).
in source:IRAS 22134+5834
Ref:=2016A&A...587A..69W
byWANG Y. , AUDARD M., FONTANI F., SANCHEZ-MONGE A., BUSQUET G., PALAU A., BEUTHER H., TAN J.C., ESTALELLA R., ISELLA A., GUETH F., JIMENEZ-SERRA I.
 Astron. Astrophys., 587A, 69-69 (2016)
  Ongoing star formation in the protocluster IRAS 22134+5834.
oFig. 1, Table 4: <[WAF2016] VLAN> (Nos VLA1-VLA2). Fig. 3, Table 6: <[WAF2016] clump> N=1, <[WAF2016] MMNa> (Nos 1-3, 3a-3b, 4-5, 5a-5b, 6). Fig. 5: <[WAF2016] HMSC6W> (Nos HMSC-E, HMSC-W).
o[PFG2013] I22134-IRS1 not in SIMBAD (no coordinates)