NGC 281-east

(NGC 281E)

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0.11 UTI
0.46
CN
0.04
Cdens
0.12
CC3
0.0
Clit
0.91
Cdup
Core radius and density 2.4 [pc], 0.2 [pc-2]
  • CN 0.46 Poorly populated
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.91 Very likely unique

Overview

â„šī¸
NGC 281-east is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below 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.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.91) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Bica et al. (2003)
Classified as infrared cluster (IRC).

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– 13.532 56.58 0.354 -2.773 -0.86 –
Lada & Lada 2003 13.561 56.556 – – – –
Bica et al. 2003 13.559 56.56 – – – –

💡 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– 2.1 – – – – 57 – –
Lada & Lada 2003 2.10 – – – – 57 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
IC 1590 8.7 13.22 56.63 0.34 -2.36 -1.49 -73.17 0.05
NGC 281 8.7 13.22 56.63 0.33 -2.36 -1.5 -67.2 0.54

💡 Note: The % column shows the percentage of members that NGC 281-east shares with each listed object.

Visualization

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