CMa02

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0.01 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.02
Cdup
Radius (P>50% members) 10.6 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.02 Very likely duplicate

Overview

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CMa02 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 105.681 -7.749 0.876 -1.59 -3.484 5.879
Hunt & Reffert 2024 105.682 -7.757 0.873 -1.576 -3.467 5.707
Cavallo et al. 2024 105.67 -7.71 0.873 – – –
Hunt & Reffert 2023 105.682 -7.757 0.873 -1.576 -3.467 5.707
Santos-Silva et al. 2021 105.68 -7.74 0.87 -1.59 -3.45 –

💡 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 – – – – – 171* – –
Cavallo et al. 2024 1.43 0.34 – 380 1.090 – – –
Hunt & Reffert 2023 1.06 0.51 0.42 239 – – – –
Santos-Silva et al. 2021 1.07* 0.99* – 137* -0.150* – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 32 98.5 105.68 -7.74 0.88 -1.59 -3.48 6.47 0.47
CWWDL 14378 77.3 105.68 -7.72 0.88 -1.58 -3.48 5.88 0.0

💡 Note: The % column shows the percentage of members that CMa02 shares with each listed object.

Visualization

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