BRC13

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0.05 UTI
0.0
CN
0.12
Cdens
0.12
CC3
0.0
Clit
0.96
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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BRC13 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) 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).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 45.192 60.603 0.342 0.056 -0.182 –
Bica et al. 2003 45.252 60.675 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
IRAS 02575+6017 40.0 45.26 60.52 0.42 -0.06 -0.09 -30.61 0.29
AFGL4029 4.0 45.21 60.54 0.44 -0.13 0.03 -30.61 0.14
IRAS 02570+6028 4.0 45.18 60.63 0.42 -0.11 0.06 -30.54 0.21
SAI 24 4.0 44.83 60.57 0.45 -0.23 0.07 -49.28 0.85

💡 Note: The % column shows the percentage of members that BRC13 shares with each listed object.

Visualization

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