ASCC 35

(MWSC 1141)

0.22 UTI

0.0

C_N

0.06

C_dens

0.12

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.12 Very 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 35 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.01 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Close Low extinction Low mass Intermediate age

Data

🔍 Search references for ASCC 35 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–	108.108	2.084	0.25	-0.552	-0.896	70.111
Just et al.	2023	108.165	2.107	–	–	–	–
Bica et al.	2019	108.166	2.123	–	–	–	–
Kharchenko et al.	2016	108.165	2.107	–	–	–	–
Dias et al.	2014	108.167	2.12	–	0.84	0.65	–
Kharchenko et al.	2013	108.172	2.105	–	-1.55	-2.25	–
Piskunov et al.	2008	108.157	2.119	–	–	–	–
Kharchenko et al.	2005	108.16	2.12	–	-2.68	-0.94	–
Dias et al.	2002	108.167	2.12	–	-2.68	-0.94	–

💡 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–	0.8	0.19	–	306	–	39	–	–
Just et al.	2023	–	–	–	302	–	39	–	–
Kharchenko et al.	2016	0.79	0.19	–	302	–	–	–	–
Kharchenko et al.	2013	0.79	0.19	–	302	–	–	–	–
Piskunov et al.	2008	0.80	0.19	–	309	–	–	–	–
Kharchenko et al.	2005	0.80	0.19	–	309	–	–	–	–
Dias et al.	2002	0.80	0.19	–	309	–	–	–	–

Visualization

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