HOPS 66
| 
 Number of sources: 2  | 
||||||||
| 
 Lbol (L⊙)  | 
 Tbol (K)  | 
 Class  | 
 Distance (pc)  | 
 Zone  | 
||||
| 
 18.3  | 
 264.9  | 
 Flat  | 
 392.8  | 
 OMC 2  | 
||||
| 
 ALMA 0.87 mm  | 
||||||||
| 
 Source  | 
 RA (J2000)  | 
 DEC (J2000)  | 
 Integrated Flux Density (mJy)  | 
 Peak Intensity (mJy/beam)  | 
 RMS (mJy/beam)  | 
 ΔΦA (")  | 
 Decon. Size (")  | 
 Decon. PA (º)  | 
| 
 HOPS-66-A  | 
 05:35:26.857  | 
 -05:09:24.40  | 
 43.31 ± 0.57  | 
 35.97  | 
 0.28  | 
 0.3  | 
 0.05 x 0.04  | 
 47  | 
| 
 HOPS-66-B  | 
 05:35:26.927  | 
 -05:09:22.43  | 
 34.62 ± 1.10  | 
 12.56  | 
 0.29  | 
 2.5  | 
 0.17 x 0.12  | 
 165.8  | 
| 
 VLA 9 mm  | 
||||||||
| 
 Source  | 
 RA (J2000)  | 
 DEC (J2000)  | 
 Integrated Flux Density (mJy)  | 
 Peak Intensity (mJy/beam)  | 
 RMS (µJy/beam)  | 
 ΔΦV (")  | 
 Decon. Size (")  | 
 Decon. PA (º)  | 
| 
 HOPS-66-A  | 
 05:35:26.857  | 
 -05:09:24.40  | 
 0.29 ± 0.01  | 
 0.25  | 
 7.96  | 
 14.7  | 
 -  | 
 -  | 
| 
 HOPS-66-B  | 
 05:35:26.927  | 
 -05:09:22.41  | 
 0.08 ± 0.01  | 
 0.07  | 
 8.01  | 
 15.2  | 
 -  | 
 -  | 
| 
 ACA 0.87 mm  | 
||||||||
| 
 Source  | 
||||||||
| 
 HOPS-66  | 
 05:35:26.832  | 
 -05:09:24.48  | 
 1000.27  | 
 298.39  | 
 8.67  | 
 -  | 
 -  | 
 -  | 
ALMA and VLA Derived Parameters
| 
 Source  | 
 R2σ, ALMA (au)  | 
 R2σ, VLA (au)  | 
 MD, ALMA (M⊕)  | 
 MD, VLA (M⊕)  | 
 QALMA  | 
 QVLA  | 
 Spectral Index (0.87 – 9 mm)  | 
 Spectral Index (8.1 -10 mm)  | 
| 
 HOPS-66-A  | 
 16.7 ± 10.0  | 
 -  | 
 19.9 ± 0.3  | 
 193.4 ± 10.1  | 
 16.58  | 
 -  | 
 2.1 ± 0.06  | 
 1.3 ± 0.41  | 
| 
 HOPS-66-B  | 
 58.0 ± 10.0  | 
 -  | 
 15.9 ± 0.5  | 
 51.5 ± 9.4  | 
 15.57  | 
 -  | 
 2.6 ± 0.09  | 
 0.5 ± 1.4  | 
Sources next/close to me: -
Same source, other names: Source 24 and 25 (Díaz-Rodríguez et al).
Source Images
Left: ALMA (0.87 mm), Right: VLA (9 mm) (Tobin et al. 2020).
Figure 1: At south west HOPS-66-A and north east HOPS-66-B.
Figure 2: HOPS-66-A.
Figure 3: HOPS-66-B.
ACA (0.87 mm) (Federman et al. 2022).

Figure 4: HOPS-66.
Source 24
| RA(J2000) | DEC(J2000) | Spectral Index | 
 Nature Evolved Stage  | 
Other Names | |||||||
| 5 cm | 3 cm | 1.3 cm | 0.7 cm | 5 cm | |||||||
| 05:35:26.9293 ± 0.0016 | -05:09:22.408 ± 0.024 | 0.26 x 0.24 | 175 ± 86 | < 0.14 | < 0.25 | 0.058 ± 0.014 | < 0.14 | 0.040 ± 0.007 | 0.29 ± 0.24 | YSO: Young Stellar Object | HOPS 66 | 
VLA (5 cm, black contours) (Díaz-Rodriguez to be submitted).

Figure 5: Source 24. Superposition of the VLA A-configuration map with natural weighting at 5cm (black contours, Díaz-Rodriguez to be submitted) over ALMA emission at 870 micron (red contours, Tobin et al 2020).
Source 25
| RA(J2000) | DEC(J2000) | Spectral Index | 
 Nature Evolved Stage  | 
Other Names | |||||||
| 5 cm | 3 cm | 1.3 cm | 0.7 cm | 5 cm | |||||||
| 05:35:26.8588 ± 0.0010 | -05:09:24.387 ± 0.015 | 0.36 x 0.06 | 106 ± 2 | < 0.14 | < 0.25 | 0.20 ± 0.03 | 0.26 ± 0.07 | 0.088 ± 0.011 | 0.57 ± 0.07 | Flat Spectrum Source | HOPS 66 | 
VLA (5 cm, black contours) (Díaz-Rodriguez to be submitted).

Figure 6: Source 25. Superposition of the VLA A-configuration map with natural weighting at 5cm (black contours, Díaz-Rodriguez to be submitted) over ALMA emission at 870 micron (red contours, Tobin et al 2020).