FSR 1595

(MWSC 1976)

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0.79 UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 87
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • 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
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FSR 1595 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Distant Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data
🔍 Search references for FSR 1595 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 – 176.77 -62.631 0.198 -6.77 1.367 -0.969
Hunt & Reffert 2024 176.768 -62.636 0.215 -6.735 1.332 -6.003
Cavallo et al. 2024 176.742 -62.611 0.214 – – –
Hunt & Reffert 2023 176.768 -62.636 0.215 -6.735 1.332 -6.003
Just et al. 2023 176.744 -62.646 – – – –
Cantat-Gaudin et al. 2020 176.771 -62.639 0.179 -6.779 1.373 –
Cantat-Gaudin & Anders 2020 176.771 -62.639 0.179 -6.779 1.373 –
Soubiran et al. 2018 176.771 -62.639 – – – -11.85
Cantat-Gaudin et al. 2018 176.771 -62.639 0.179 -6.779 1.373 –
Kharchenko et al. 2016 176.744 -62.646 – – – –
Dias et al. 2014 176.771 -62.637 – -8.46 -2.82 –
Kharchenko et al. 2013 176.752 -62.65 – -3.48 -1.28 0.0
Froebrich et al. 2007 176.771 -62.637 – – – –
Dias et al. 2002 176.771 -62.637 – -3.48 -1.28 –

💡 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 – – – – – 843* – –
Cavallo et al. 2024 3.77 3.24 – 89 -0.040 – – –
Hunt & Reffert 2023 4.06 2.92 2.53 48 – – – –
Just et al. 2023 – – – 2 – 822 – –
Cantat-Gaudin et al. 2020 5.40 2.45 – 692 – – – –
Cantat-Gaudin & Anders 2020 4.81 – – – – – – –
Soubiran et al. 2018 4.81 – – – – – – –
Cantat-Gaudin et al. 2018 4.81 – – – – – – –
Kharchenko et al. 2016 4.42 2.65 – 2 – – – –
Kharchenko et al. 2013 4.42 2.65 – 2 – – – –
Dias et al. 2002 4.42 2.65 – 2 – – – –

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

Visualization
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FSR 1595 UCC
FSR 1595 HUNT23
FSR 1595 CANTAT20
Galactocentric position diagram