Teutsch 14b

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0.10 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.18
Cdup
Stellar density (N50/rad) 42.7 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.18 Likely duplicate

Overview

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Teutsch 14b is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

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

(*): The parallax distance estimate (~3.19 kpc) differs significantly from the median photometric distance (~1.72 kpc).

Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 270.876 -22.129 0.314 -0.38 -1.672 31.142
Morales et al. 2013 270.884 -22.138 – – – –
Kronberger et al. 2006 270.884 -22.138 – – – –

💡 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– 1.72 – – – – – – –
Morales et al. 2013 1.72 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 14a 81.5 270.87 -22.13 0.32 -0.35 -1.65 22.06 0.75

💡 Note: The % column shows the percentage of members that Teutsch 14b shares with each listed object.

Visualization

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