Hogg 9

(MWSC 1874; OCL 832; ESO 128 24)

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0.14 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.29
Clit
1.0
Cdup
Core radius and density 3.3 [pc], 0.09 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
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).

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

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 – – – –
Sampedro et al. 2017 164.592 -59.05 – 0.4 -1.32 –
Joshi et al. 2016 164.602 -59.053 – – – –
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 –
Bukowiecki et al. 2011 164.6 -59.053 – – – –
Dias et al. 2002 164.592 -59.05 – 0.12 -0.97 –
Lynga 1987 164.601 -59.054 – – – –

💡 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] Bfrac BSS
UCC 99999– 1.75 1.31 – 79 – 300 – –
Just et al. 2023 – – – 79 – 74 – –
Joshi et al. 2016 1.75 1.31 – 79 – – – –
Kharchenko et al. 2016 1.75 1.31 – 79 – – – –
Kharchenko et al. 2013 1.75 1.31 – 79 – – – –
Bukowiecki et al. 2012 – – – – – 525 – –
Bukowiecki et al. 2011 3.06(1) 1.17 – 28 – – – –
Dias et al. 2002 3.05 1.20 – 28 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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