NGC 2175

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0.78 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members) 7.0 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.7 Moderately studied
  • Cdup 1.0 Unique

Overview

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NGC 2175 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 92.404 20.597 0.501 0.289 -2.263 23.039
Hunt & Reffert 2024 92.349 20.636 0.512 0.386 -2.246 23.043
Cavallo et al. 2024 92.51 20.556 0.517 – – –
Hunt & Reffert 2023 92.349 20.636 0.512 0.386 -2.246 23.043
Jaehnig et al. 2021 92.433 20.562 0.513 0.419 -2.33 –
Loktin & Popova 2017 92.415 20.487 – 0.382 -2.656 22.0
Dias et al. 2014 92.412 20.487 – 0.37 -5.39 –
Gozha et al. 2012 92.413 20.487 – – – –
Kharchenko et al. 2007 92.41 20.49 – 0.18 – –
van den Bergh 2006 92.425 20.5 – – – –
Chen et al. 2003 92.417 20.309 – 1.8 -2.26 22.0
Dias et al. 2002 92.412 20.487 – 1.8 -2.26 23.2
Dambis 1999 92.412 20.487 – – – –

💡 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 – – – – – 229* – –
Cavallo et al. 2024 1.78 1.73 – 7 -0.300 – – –
Hunt & Reffert 2023 1.79 1.49 1.89 6 – – – –
Jaehnig et al. 2021 2.00* – – – – – – –
Loktin & Popova 2017 1.62 1.82 – 9 – – – –
Gozha et al. 2012 1.63 – – 9 – – – –
van den Bergh 2006 1.63 1.86 – 9 – – – –
Chen et al. 2003 1.63 – – 0 – – – –
Dias et al. 2002 1.63 1.85 – 9 – – – –
Dambis 1999 1.79 2.41 – 3 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Pismis 27 6.9 92.73 20.62 0.51 -0.19 -2.05 32.5 0.83

💡 Note: The % column shows the percentage of members that NGC 2175 shares with each listed object.

Visualization

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