ASCC 37

(MWSC 1169)

0.28 UTI

0.0

C_N

0.1

C_dens

0.38

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 0.5 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.38 Low quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ASCC 37 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.79 kpc) differs significantly from the median photometric distance (~1.60 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for ASCC 37 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–	109.544	-24.475	0.173	-1.156	2.486	–
Just et al.	2023	109.509	-24.497	–	–	–	–
Bica et al.	2019	109.52	-24.478	–	–	–	–
Kharchenko et al.	2016	109.509	-24.497	–	–	–	–
Dias et al.	2014	109.517	-24.48	–	-1.71	3.61	–
Kharchenko et al.	2013	109.515	-24.5	–	-2.44	1.59	13.5
Piskunov et al.	2008	109.511	-24.482	–	–	–	–
Kharchenko et al.	2005	109.51	-24.48	–	-3.04	0.81	–
Dias et al.	2002	109.517	-24.48	–	-1.71	3.61	13.5

💡 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–	1.6	0.0	–	537	–	88	–	–
Just et al.	2023	–	–	–	537	–	88	–	–
Kharchenko et al.	2016	1.57	0.39	–	537	–	–	–	–
Kharchenko et al.	2013	1.57	0.39	–	537	–	–	–	–
Piskunov et al.	2008	1.60	0.00	–	537	–	–	–	–
Kharchenko et al.	2005	1.60	0.00	–	537	–	–	–	–
Dias et al.	2002	1.60	0.00	–	537	–	–	–	–

Visualization

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