Ruprecht 115

(MWSC 2368)

Click to load Aladin Lite
0.95 UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 130
Stellar density (N50/rad) 45.4 [N/pc2]
C3 classification AA
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very 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
Ruprecht 115 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.

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

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for Ruprecht 115 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 243.213 -52.396 0.378 -4.353 -4.556 -41.183
Hunt & Reffert 2024 243.214 -52.397 0.39 -4.313 -4.587 -39.897
Cavallo et al. 2024 243.217 -52.397 0.39 – – –
Hunt & Reffert 2023 243.214 -52.397 0.39 -4.313 -4.587 -39.897
Just et al. 2023 243.228 -52.426 – – – –
Jaehnig et al. 2021 243.214 -52.392 0.382 -4.371 -4.569 –
Rain et al. 2021 243.215 -52.393 0.366 -4.333 -4.546 –
Cantat-Gaudin et al. 2020 243.215 -52.393 0.366 -4.333 -4.546 –
SΓ‘nchez et al. 2020 243.217 -52.4 – -4.4 -4.397 –
Cantat-Gaudin & Anders 2020 243.215 -52.393 0.366 -4.333 -4.546 –
Bossini et al. 2019 243.215 -52.393 – – – –
Soubiran et al. 2018 243.215 -52.393 – – – -40.5
Cantat-Gaudin et al. 2018 243.215 -52.393 0.366 -4.333 -4.546 –
Kharchenko et al. 2016 243.228 -52.426 – – – –
Dias et al. 2014 243.217 -52.4 – -2.49 -4.8 –
Kharchenko et al. 2013 243.24 -52.427 – -3.73 -6.26 –
Morales et al. 2013 243.217 -52.4 – – – –
Bukowiecki et al. 2011 243.208 -52.391 – – – –
van den Bergh 2006 243.2 -52.383 – – – –
Dias et al. 2002 243.217 -52.4 – -2.49 -4.8 –

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– 2.35 2.285 1.83 582 -0.102 668 – 0.0
Hunt & Reffert 2024 – – – – – 954(1) – –
Cavallo et al. 2024 1.79 3.56 – 112 -0.600 – – –
Hunt & Reffert 2023 2.35 2.96 1.83 157 – – – –
Just et al. 2023 – – – 1365 – 116 – –
Jaehnig et al. 2021 2.59(1) – – – – – – –
Rain et al. 2021 2.53 2.02 – 603 – – – 0
Cantat-Gaudin et al. 2020 2.36 2.25 – 234 – – – –
Cantat-Gaudin & Anders 2020 2.53 – – – – – – –
Bossini et al. 2019 2.41 2.32 – 298 -0.102 – – –
Soubiran et al. 2018 2.53 – – – – – – –
Cantat-Gaudin et al. 2018 2.53 – – – – – – –
Kharchenko et al. 2016 1.95 2.90 – 1365 – – – –
Kharchenko et al. 2013 1.95 2.90 – 1365 – – – –
Morales et al. 2013 2.00 – – 398 – – – –
Bukowiecki et al. 2012 – – – – – 668 – –
Bukowiecki et al. 2011 2.29(1) 1.92 – 562 – – – –
van den Bergh 2006 2.16 2.02 – 603 – – – –
Dias et al. 2002 2.16 2.02 – 603 0.040 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0646 21.5 243.21 -52.39 0.4 -4.36 -4.53 -39.97 0.0

πŸ’‘ Note: The % column shows the percentage of members that Ruprecht 115 shares with each listed object.

Visualization
ℹ️
Ruprecht 115 UCC
Ruprecht 115 HUNT23
Ruprecht 115 CANTAT20
Galactocentric position diagram