BDB2003 G045.45+00.06

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0.02 UTI
0.46
CN
0.03
Cdens
0.38
CC3
0.0
Clit
0.11
Cdup
Nm (P>50%) 46
Core radius and density 6.1 [pc], 0.1 [pc-2]
C3 classification BC
  • CN 0.46 Poorly populated
  • Cdens 0.03 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.11 Likely duplicate
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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BDB2003 G045.45+00.06 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large 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.

⚠ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. 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
🔍 Search references for BDB2003 G045.45+00.06 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 288.619 11.131 0.121 -2.644 -5.489 42.971
Morales et al. 2013 288.587 11.153 – – – –

💡 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– 6.66 – – – – – – –
Morales et al. 2013 6.66 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
G45.45+0.06 89.1 288.62 11.12 0.12 -2.64 -5.49 53.3 0.17
BDSB 136 30.4 288.62 11.16 0.21 -2.73 -5.8 63.62 0.04

💡 Note: The % column shows the percentage of members that BDB2003 G045.45+00.06 shares with each listed object.

Visualization
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BDB2003 G045.45+00.06 UCC
Galactocentric position diagram