Haffner 24

(MWSC 1239; OCL 608; ESO 559 14)

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0.33 UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Haffner 24 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.49 kpc) differs significantly from the median photometric distance (~2.23 kpc).

Relatively close Moderate extinction Very metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 112.174 -18.297 0.287 -1.631 2.124 70.914
Hunt & Reffert 2024 112.166 -18.27 0.295 -1.634 2.136 70.885
Cavallo et al. 2024 112.143 -18.288 0.294 – – –
Hunt & Reffert 2023 112.166 -18.27 0.295 -1.634 2.136 70.885
Just et al. 2023 112.231 -18.313 – – – –
Bica et al. 2019 112.22 -18.344 – – – –
Kharchenko et al. 2016 112.231 -18.313 – – – –
Kharchenko et al. 2013 112.237 -18.315 – -2.52 6.63 –
Dias et al. 2002 112.233 -18.317 – -2.52 6.63 –

💡 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
Hunt & Reffert 2024 – – – – – 233* – –
Cavallo et al. 2024 2.23 1.60 – 229 -1.000 – – –
Hunt & Reffert 2023 3.10 1.07 0.61 275 – – – –
Just et al. 2023 – – – 343 – 32 – –
Kharchenko et al. 2016 1.71 0.84 – 343 – – – –
Kharchenko et al. 2013 1.71 0.84 – 343 – – – –
Dias et al. 2002 2.94 1.49 – 79 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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