Hogg 9

(MWSC 1874; OCL 832; ESO 128 24)

0.18 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 14

Radius (P>50% members) 6.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Hogg 9 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.51 kpc) differs significantly from the median photometric distance (~1.75 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Young

Data

🔍 Search references for Hogg 9 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	164.543	-59.096	0.222	-7.256	2.657	–
Just et al.	2023	164.595	-59.049	–	–	–	–
Bica et al.	2019	164.593	-59.063	–	–	–	–
Kharchenko et al.	2016	164.595	-59.049	–	–	–	–
Dias et al.	2014	164.592	-59.05	–	0.34	-1.07	–
Kharchenko et al.	2013	164.602	-59.053	–	-4.77	4.58	–
Dias et al.	2002	164.592	-59.05	–	0.12	-0.97	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Just et al.	2023	–	–	–	79	–	74	–	–
Kharchenko et al.	2016	1.75	1.29	–	79	–	–	–	–
Kharchenko et al.	2013	1.75	1.29	–	79	–	–	–	–
Dias et al.	2002	3.05	1.18	–	28	–	–	–	–

Visualization

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