HOPS 182

Number of components: 3

Lbol (L)

Tbol (K)

Class

Distance (pc)

Zone

59.8

51.9

0

385.1

LDN 1641

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-182-A

05:36:18.795

-06:22:10.21

741.93 ± 8.0

97.73

1.63

0.6

0.21 x 0.16

150.8

HOPS-182-B

05:36:18.775

-06:22:11.15

111.17 ± 4.1

71.78

1.65

1.3

0.11 x 0.06

79.4

HOPS-182-C

05:36:18.478

-06:22:13.62

17.03 ± 3.4

13.77

2.29

6.3

0.07 x 0.04

127.1

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-182-A

05:36:18.797

-06:22:10.23

0.72 ± 0.03

0.30

7.4

0.5

0.12 x 0.09

10.2

HOPS-182-B

05:36:18.776

-06:22:11.17

1.22 ± 0.02

0.80

7.41

1.3

0.06 x 0.05

86.4

HOPS-182-C

05:36:18.480

-06:22:13.64

0.17 ± 0.02

0.13

7.52

6.3

0.06 x 0.03

162.1

ACA 0.87 mm

Source

RA

(J2000)

DEC

(J2000)

Integrated Flux Density

(mJy)

Peak Intensity

(mJy/beam)

RMS

(mJy/beam)

ΔΦV

(")

Decon. Size

(")

Decon. PA

(º)

HOPS-182

05:36:18.84

-06:22:10.2

2395.9

1341.57

13.06

-

-

-

 

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-182-A

69.7 ± 10.0

38.3 ± 10.0

238.1 ± 2.6

338.7 ± 13.7

0.72

0.64

3.0 ± 0.06

3.0 ± 0.36

HOPS-182-B

36.3 ± 10.0

20.3 ± 10.0

35.7 ± 1.3

576.2 ± 9.0

5.65

0.42

1.9 ± 0.06

1.2 ± 0.13

HOPS-182-C

21.3 ± 12.8

18.0 ± 10.0

5.5 ± 1.5

80.1 ± 7.7

41.63

3.05

2.0 ± 0.11

2.5 ± 0.83

 


Sources next/close to me: -

Same source, other names: -


 

Source Images

Left: ALMA (0.87 mm), Right: VLA (9 mm) (Tobin et al. 2020).

Figure 1: HOPS-182-A at north east, HOPS-182-B below and HOPS-182-C at south west.

 

Figure 2: HOPS-182-A at north east and HOPS-182-B at south west.

 

Figure 3: HOPS-182-C.

 

ACA (0.87 mm) (Federman et al. 2022).

Figure 4: HOPS-182.