Hogg 12

(MWSC 1918; OCL 851; ESO 129 11)

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0.37 UTI
0.28
CN
0.05
Cdens
0.5
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.05 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Hogg 12 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~7.84 kpc) differs significantly from the median photometric distance (~1.66 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Low mass Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 168.059 -60.772 0.128 -5.541 1.998 7.429
Just et al. 2023 168.052 -60.761 – – – –
SΓ‘nchez et al. 2020 168.254 -60.783 – -6.234 1.005 –
Bica et al. 2019 168.066 -60.755 – – – –
Kharchenko et al. 2016 168.052 -60.761 – – – –
Dias et al. 2014 168.254 -60.783 – -3.43 -1.84 –
Kharchenko et al. 2013 168.06 -60.765 – -7.04 1.34 -3.0
Kharchenko et al. 2003 168.07 -60.75 – -8.99 2.0 –
Dias et al. 2002 168.254 -60.783 – -3.43 -1.84 –

πŸ’‘ 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 – – – 40 – 20 – –
Kharchenko et al. 2016 1.66 1.24 – 40 – – – –
Kharchenko et al. 2013 1.66 1.24 – 40 – – – –
Kharchenko et al. 2003 1.43 0.93 – – – – – –
Dias et al. 2002 2.00 1.24 – 30 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4456 50.0 168.03 -60.77 0.13 -5.66 2.0 – 0.04

πŸ’‘ Note: The % column shows the percentage of members that Hogg 12 shares with each listed object.

Visualization

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