IC 1590

Click to load Aladin Lite
0.91 UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 249
Stellar density (N50/rad) 34.5 [N/pc2]
C3 classification AB
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 MOCAMOCA πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
IC 1590 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is very well-studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Cavallo et al. (2024)
Silver sample.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.

Data
πŸ” Search references for IC 1590 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 13.217 56.629 0.336 -2.363 -1.486 -73.169
Almeida et al. 2025 13.202 56.629 – – – –
Hunt & Reffert 2024 13.207 56.632 0.333 -2.367 -1.467 -59.698
Celli et al. 2024 13.205 56.629 – – – –
Cavallo et al. 2024 13.242 56.619 0.336 – – –
Hunt & Reffert 2023 13.207 56.632 0.333 -2.367 -1.467 -59.698
Almeida et al. 2023 13.215 56.633 – – – –
Dias et al. 2021 13.202 56.629 0.343 -2.373 -1.452 –
Cantat-Gaudin et al. 2020 13.205 56.629 0.339 -2.368 -1.449 –
SΓ‘nchez et al. 2020 13.204 56.628 – -2.605 -1.465 –
Zhong et al. 2020 13.205 56.629 – -2.368 -1.449 83.202
Cantat-Gaudin & Anders 2020 13.205 56.629 0.339 -2.368 -1.449 –
Cantat-Gaudin et al. 2018 13.205 56.629 0.339 -2.368 -1.449 –
Loktin & Popova 2017 13.2 56.628 – -0.263 -3.618 -32.5
Dias et al. 2014 13.204 56.628 – -2.43 -1.9 –
Gozha et al. 2012 13.204 56.628 – – – –
Bukowiecki et al. 2011 13.192 56.619 – – – –
Piskunov et al. 2008 13.199 56.631 – – – –
Kharchenko et al. 2007 13.2 56.63 – 0.11 – -32.46
van den Bergh 2006 13.2 56.633 – – – –
Kharchenko et al. 2005 13.2 56.63 – -1.36 -1.34 -37.5
Dias et al. 2002 13.204 56.628 – -2.43 -1.9 -25.16

πŸ’‘ 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– 2.605 0.99 2.57 7 -0.157 609 0.78 –
Almeida et al. 2025 2.35 1.27 – 11 – 403 – –
Hunt & Reffert 2024 – – – – – 1059(1) – –
Celli et al. 2024 – – – 6 – 567 – –
Cavallo et al. 2024 2.10 0.90 – 17 -0.240 – – –
Hunt & Reffert 2023 2.73 1.57 2.57 12 – – – –
Almeida et al. 2023 2.53 1.31 – 7 -0.128 651(1) 0.78 –
Dias et al. 2021 2.35 1.27 – 11 -0.157 – – –
Cantat-Gaudin et al. 2020 2.98 1.13 – 6 – – – –
Zhong et al. 2020 0.00 0.00 – 0 0.000 – – –
Cantat-Gaudin & Anders 2020 2.72 – – – – – – –
Cantat-Gaudin et al. 2018 2.72 – – – – – – –
Loktin & Popova 2017 2.38 0.99 – 11 – – – –
Bukowiecki et al. 2012 – – – – – 1055 – –
Gozha et al. 2012 2.94 – – 3 -0.730 52 – –
Bukowiecki et al. 2011 2.68(1) 1.21 – 7 – – – –
Piskunov et al. 2008 2.38 0.99 – 7 – – – –
van den Bergh 2006 2.94 0.99 – 3 – – – –
Kharchenko et al. 2005 2.38 0.99 – 7 – – – –
Dias et al. 2002 2.94 0.99 – 3 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 281 93.6 13.22 56.63 0.33 -2.36 -1.5 -67.2 0.12
NGC 281W 51.4 13.2 56.62 0.34 -2.36 -1.52 -73.41 0.02

πŸ’‘ Note: The % column shows the percentage of members that IC 1590 shares with each listed object.

Visualization
ℹ️
IC 1590 UCC
IC 1590 HUNT23
IC 1590 CANTAT20
Galactocentric position diagram