NGC 281-west

(NGC 281W)

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0.01 UTI
0.71
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.01
Cdup
Core radius and density 1.4 [pc], 5.9 [pc-2]
  • CN 0.71 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.01 Very likely duplicate

Overview

â„šī¸
NGC 281-west is a moderately populated, very dense object of very high 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.

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.

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– 13.186 56.622 0.339 -2.379 -1.511 -73.406
Lada & Lada 2003 13.099 56.562 – – – –
Bica et al. 2003 13.091 56.572 – – – –

💡 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 – – – – 130 – –
Lada & Lada 2003 2.10 – – – – 130 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 281 98.9 13.22 56.63 0.33 -2.36 -1.5 -67.2 0.54
IC 1590 97.8 13.22 56.63 0.34 -2.36 -1.49 -73.17 0.05

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

Visualization

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