HOPS 64
| 
 Distance (pc)  | 
 Zone  | 
|||||||
| 
 13.4  | 
 29.7  | 
 I  | 
 392.8  | 
 OMC 2  | 
||||
| 
 ALMA 0.87 mm  | 
||||||||
| 
 Source  | 
||||||||
| 
 HOPS-64  | 
 05:35:26.998  | 
 -05:09:57.08  | 
 33.47 ± 0.76  | 
 20.37  | 
 0.41  | 
 6.4  | 
 0.1 x 0.07  | 
 119.3  | 
| 
 VLA 9 mm  | 
||||||||
| 
 Source  | 
||||||||
| 
 HOPS-64  | 
 05:35:26.966  | 
 -05:09:54.08  | 
 0.26 ± 0.02  | 
 0.17  | 
 7.12  | 
 6.4  | 
 0.06 x 0.05  | 
 158.6  | 
| 
 ACA 0.87 mm  | 
||||||||
| 
 Source  | 
||||||||
| 
 HOPS-64  | 
 -  | 
 -  | 
 -  | 
 -  | 
 -  | 
 -  | 
 -  | 
 -  | 
ALMA and VLA Derived Parameters
| 
 Source  | 
||||||||
| 
 HOPS-64  | 
 31.7 ± 10.0  | 
 19.7 ± 10.0  | 
 16.8 ± 0.5  | 
 182.1 ± 13.1  | 
 18.62  | 
 1.93  | 
 2.1 ± 0.07  | 
 2.5 ± 0.61  | 
Sources next/close to me: HOPS-108, VLA-16.
Same source, other names: FIR 4d/e, MIPS 2293.
Source Images
Left: ALMA (0.87 mm), Right: VLA (9 mm) (Tobin et al. 2020).
Figure 1: HOPS-64.
Figure 2: At north west HOPS-64 and south east HOPS-108.
Figure 3: At the top HOPS-64, at middle east HOPS-108 and south west VLA16.
HOPS-64
(from Osorio et al. 2017)
| RA(J2000) | DEC(J2000) | Spectral Index | 
 Nature Evolved Stage  | 
Other Names | ||||||
| 5 cm | 3 cm | 1.3 cm | 0.9 cm | 0.7 cm | ||||||
| 05:35:26.9960 ± 0.0023 | -05:09:54.06 ± 0.03 | - | 0.011 ± 0.003 | < 0.03 | 0.069 ± 0.012 | 0.140 ± 0.016 | 1.51 ± 0.060 | - | Class I | MIPS 2293, MIR 24, FIR 4d/e | 
VLA (5 cm, 3 cm, 1.3 cm, 0.9 cm and 0.7 cm) (Osorio et al. 2017).

Figure 1: Entire sources map. HOPS-64 emission at 1.3 cm and 0.7 cm.