Carraro 1

(MWSC 1829)

0.30 UTI

0.36

C_N

0.08

C_dens

0.25

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification CC

C_N 0.36 Poorly populated
C_dens 0.08 Very loose
C_C3 0.25 Low quality
C_lit 0.4 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

Carraro 1 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.12 kpc) differs significantly from the median photometric distance (~1.84 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Low mass Old

Data

🔍 Search references for Carraro 1 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	159.274	-58.732	0.32	-5.984	2.399	–
Just et al.	2023	159.226	-58.746	–	–	–	–
Bica et al.	2019	159.238	-58.753	–	–	–	–
Kharchenko et al.	2016	159.226	-58.746	–	–	–	–
Dias et al.	2014	159.25	-58.733	–	-6.74	-2.51	–
Kharchenko et al.	2013	159.232	-58.75	–	-7.11	-2.01	-8.5
van den Bergh	2006	159.25	-58.733	–	–	–	–
Dias et al.	2002	159.25	-58.733	–	-6.74	-2.51	-8.5

💡 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]	B_frac	BSS
UCC	99999–	1.845	0.81	–	1259	–	16	–	–
Just et al.	2023	–	–	–	1259	–	16	–	–
Kharchenko et al.	2016	1.79	0.84	–	1259	–	–	–	–
Kharchenko et al.	2013	1.79	0.84	–	1259	–	–	–	–
van den Bergh	2006	1.90	0.78	–	3020	–	–	–	–
Dias et al.	2002	1.90	0.78	–	3020	–	–	–	–

Visualization

ℹ️