ASCC 60

(MWSC 1823)

Click to load Aladin Lite
0.49 UTI
0.0
CN
0.18
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 17
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.75 High quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
ASCC 60 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~5.46 kpc) differs significantly from the median photometric distance (~0.96 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data
🔍 Search references for ASCC 60 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 158.173 -58.62 0.183 -5.441 2.588 109.416
Hunt & Reffert 2024 158.171 -58.631 0.187 -5.436 2.595 109.321
Cavallo et al. 2024 158.191 -58.59 0.185 – – –
Hunt & Reffert 2023 158.171 -58.631 0.187 -5.436 2.595 109.321
Just et al. 2023 158.281 -58.478 – – – –
Bica et al. 2019 158.27 -58.482 – – – –
Kharchenko et al. 2016 158.281 -58.478 – – – –
Dias et al. 2014 158.279 -58.48 – -3.97 -3.26 –
Kharchenko et al. 2013 158.287 -58.482 – -7.86 3.87 -14.5
Gozha et al. 2012 158.279 -58.48 – – – –
Piskunov et al. 2008 158.28 -58.477 – – – –
Kharchenko et al. 2007 158.28 -58.48 – 0.12 – -14.5
Kharchenko et al. 2005 158.28 -58.48 – -7.35 2.36 -14.5
Dias et al. 2002 158.279 -58.48 – -3.97 -3.26 37.0

💡 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 – – – – – 935* – –
Cavallo et al. 2024 3.52 3.38 – 38 -0.490 – – –
Hunt & Reffert 2023 4.55 2.63 3.13 46 – – – –
Just et al. 2023 – – – 133 – 77 – –
Kharchenko et al. 2016 1.12 0.48 – 133 – – – –
Kharchenko et al. 2013 1.12 0.48 – 133 – – – –
Gozha et al. 2012 0.80 – – 229 – 19 – –
Piskunov et al. 2008 0.80 0.31 – 229 – – – –
Kharchenko et al. 2005 0.80 0.31 – 229 – – – –
Dias et al. 2002 0.80 0.31 – 229 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2275 84.0 158.18 -58.62 0.2 -5.47 2.56 85.96 0.37

💡 Note: The % column shows the percentage of members that ASCC 60 shares with each listed object.

Visualization
ℹī¸
ASCC 60 UCC
ASCC 60 HUNT23
Galactocentric position diagram