AH03 J2011+26.7

(MWSC 3281)

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0.52 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 6.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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AH03 J2011+26.7 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a relatively close* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~1.66 kpc) differs significantly from the median photometric distance (~3.12 kpc).

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 302.923 26.617 0.601 -3.196 -5.662 -29.059
Bica et al. 2019 302.988 26.738 – – – –
Dias et al. 2014 302.987 26.736 – 0.29 -2.56 –
Bukowiecki et al. 2011 302.962 26.734 – – – –
Dias et al. 2002 302.988 26.736 – 0.29 -2.56 –

💡 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– 3.115 2.76 – 22 – 116 – –
Bukowiecki et al. 2012 – – – – – 116 – –
Bukowiecki et al. 2011 3.66(1) 2.73 – 22 – – – –
Dias et al. 2002 2.57 2.79 – 22 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 18 100.0 302.91 26.54 0.61 -3.21 -5.66 -3.42 0.79

💡 Note: The % column shows the percentage of members that AH03 J2011+26.7 shares with each listed object.

Visualization

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