Can-Battlo 1

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0.10 UTI
0.5
CN
0.86
Cdens
0.62
CC3
0.0
Clit
0.24
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.86 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

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Can-Battlo 1 is a moderately populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš 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.

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 68.557 45.45 0.316 -0.253 -1.06 -2.121
Hunt & Reffert 2024 68.556 45.457 0.337 -0.266 -1.08 –
Cavallo et al. 2024 68.567 45.45 0.33 – – –
Hunt & Reffert 2023 68.556 45.457 0.337 -0.266 -1.08 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 195* – –
Cavallo et al. 2024 3.15 2.98 – 63 -0.090 – – –
Hunt & Reffert 2023 2.88 2.75 1.71 91 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1607 76.0 68.56 45.45 0.32 -0.28 -1.07 -2.12 0.31

💡 Note: The % column shows the percentage of members that Can-Battlo 1 shares with each listed object.

Visualization

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