BDB2003 G012.80-00.19

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0.48 UTI
0.39
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 11.3 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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BDB2003 G012.80-00.19 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near 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 13 years.

(*): The parallax distance estimate (~2.56 kpc) differs significantly from the median photometric distance (~3.79 kpc).

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded, presence of emission related to PAH or warm dust.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 273.512 -17.988 0.391 -1.189 -3.117 -1.522
Morales et al. 2013 273.554 -17.932 – – – –

💡 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– 3.79 – – – – – – –
Morales et al. 2013 3.79 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 161 94.9 273.51 -18.0 0.39 -1.19 -3.12 -2.72 0.0
MDF2011 cl2 94.9 273.51 -18.0 0.39 -1.17 -3.12 -2.83 0.43

💡 Note: The % column shows the percentage of members that BDB2003 G012.80-00.19 shares with each listed object.

Visualization

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