IRAS 00013+6817

(MWSC 9)

Click to load Aladin Lite
0.06 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.1
Clit
0.96
Cdup
Nm (P>50%) 21
Core radius and density 6.5 [pc], 0.06 [pc-2]
C3 classification DC
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.1 Rarely studied
  • Cdup 0.96 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
IRAS 00013+6817 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~5.96 kpc) differs significantly from the median photometric distance (~1.34 kpc).

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

⚠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.

Data
🔍 Search references for IRAS 00013+6817 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 0.756 68.55 0.168 -1.655 -0.501 -97.8
Just et al. 2023 0.987 68.562 – – – –
Joshi et al. 2016 0.996 68.565 – – – –
Kharchenko et al. 2016 0.987 68.562 – – – –
Kharchenko et al. 2013 0.996 68.565 – -3.52 -1.55 –
Kharchenko et al. 2012 0.996 68.565 – -3.52 -1.55 –

💡 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– 1.34 2.63 – 14 – 52 – –
Just et al. 2023 – – – 14 – 52 – –
Joshi et al. 2016 1.34 2.63 – 14 – – – –
Kharchenko et al. 2016 1.34 2.63 – 14 – – – –
Kharchenko et al. 2013 1.34 2.63 – 14 – – – –
Kharchenko et al. 2012 1.34 2.63 – 14 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BRC2 4.0 0.93 68.49 0.13 -1.69 0.03 -85.17 0.08

💡 Note: The % column shows the percentage of members that IRAS 00013+6817 shares with each listed object.

Visualization
ℹī¸
IRAS 00013+6817 UCC
Galactocentric position diagram