NGC 7438

(FSR 0380; MWSC 3682)

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0.52 UTI
0.0
CN
0.22
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members) 19.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.75 High quality
  • Clit 0.82 Well-studied
  • Cdup 1.0 Unique

Overview

NGC 7438 is a sparse, very loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Close Moderate extinction Near-solar metallicity Intermediate age

Hunt & Reffert (2024): Classified as a moving group.

Cavallo et al. (2024): Gold sample.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 344.793 54.322 1.209 -2.275 -4.264 -34.759
Zhang et al. 2024 344.671 54.251
Cavallo et al. 2024 345.645 54.546 1.227
Hunt & Reffert 2023 344.671 54.251 1.231 -2.204 -4.247 -37.127
Just et al. 2023 344.333 54.371
Bica et al. 2019 344.327 54.357
Loktin & Popova 2017 344.34 54.339 -0.535 -0.535 -17.0
Kharchenko et al. 2016 344.333 54.371
Kharchenko et al. 2013 344.34 54.375 0.01 -1.55 -17.0
Kharchenko et al. 2012 344.34 54.375 0.01 -1.55 -17.0
Piskunov et al. 2008 344.326 54.335
Kharchenko et al. 2007 344.34 54.34 0.23 -17.0
Piskunov et al. 2007 344.326 54.335
Froebrich et al. 2007 344.146 54.251
Kharchenko et al. 2005 344.34 54.34 1.53 -1.18

💡 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
Zhang et al. 2024 0.005*
Cavallo et al. 2024 0.83 0.92 269 0.460
Hunt & Reffert 2023 0.77 0.81 0.32 238
Just et al. 2023 631 92
Loktin & Popova 2017 2.08 0.28 631
Kharchenko et al. 2016 1.00 1.08 631
Kharchenko et al. 2013 1.00 1.08 631
Kharchenko et al. 2012 1.00 1.08 631
Piskunov et al. 2008 0.60 1.24 851 121*
Piskunov et al. 2007 0.60 1.24 851 22
Kharchenko et al. 2005 0.60 1.24 851

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.