Ferrero 38

0.33 UTI

0.64

C_N

0.27

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 79

Core radius and density 1.9 [pc], 1.3 [pc^-2]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 0.27 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Ferrero 38 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

Note: This object shares a significant percentage of members with 4 later reported entries. See table with shared members information.

No fundamental parameters

Bica et al. (2019)
Asterisms and clusters by L. Ferrero.

Data

🔍 Search references for Ferrero 38 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	99999–	37.57	59.791	0.342	-0.092	-0.492	-51.172
Bica et al.	2019	37.627	59.769	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 190	62.0	37.43	59.79	0.34	-0.07	-0.49	–	0.08
CWWDL 2007	58.2	37.43	59.78	0.35	-0.06	-0.49	–	0.05
OC 0249	26.6	37.37	59.83	0.35	-0.07	-0.46	–	0.03
CWWDL 8509	5.1	37.29	59.48	0.37	-0.03	-0.59	–	0.06

💡 Note: The % column shows the percentage of members that Ferrero 38 shares with each listed object.

Visualization

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