Delta Cephei Cluster

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0.50 UTI
0.66
CN
0.83
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 62.7 [arcmin]
  • CN 0.66 Moderately populated
  • Cdens 0.83 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Delta Cephei Cluster is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 335.467 56.638 4.139 16.9 4.724 -14.536
Cavallo et al. 2024 334.358 56.042 4.113 – – –
Hunt & Reffert 2023 336.424 57.157 4.113 16.506 4.667 -15.482
Bica et al. 2019 335.634 56.565 – – – –

💡 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
Cavallo et al. 2024 0.25 0.51 – 36 0.070 – – –
Hunt & Reffert 2023 0.24 0.07 0.43 67 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 33 79.0 335.08 56.53 4.13 16.79 4.81 -13.98 0.06
Cep OB6 30.9 335.13 56.44 4.13 16.79 4.79 -14.34 0.0

💡 Note: The % column shows the percentage of members that Delta Cephei Cluster shares with each listed object.

Visualization

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