Cep A

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0.03 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.08
Cdup
Stellar density (N50/rad) 8.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

â„šī¸
Cep A is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 344.049 62.055 1.251 -0.98 -2.644 -20.625
Lada & Lada 2003 344.079 62.032 – – – –

💡 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] Bfrac BSS
UCC 99999– 0.7 – – – – 310 – –
Lada & Lada 2003 0.70 – – – – 310 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Cepheus A 92.0 344.05 62.06 1.25 -1.05 -2.64 -20.62 0.28

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

Visualization

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