ASCC 26

(MWSC 995)

0.27 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.6

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 13

Radius (P>50% members) 8.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very low quality
C_lit 0.6 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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ASCC 26 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 moderately studied in the literature.

(*): The parallax distance estimate (~3.40 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Close Low extinction Low mass Intermediate age

Data

🔍 Search references for ASCC 26 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	–	102.594	7.245	0.294	-0.338	-0.465	–
Just et al.	2023	102.6	7.252	–	–	–	–
Bica et al.	2019	102.598	7.255	–	–	–	–
Kharchenko et al.	2016	102.6	7.252	–	–	–	–
Dias et al.	2014	102.6	7.25	–	-0.73	-3.14	–
Kharchenko et al.	2013	102.607	7.25	–	-3.01	-2.09	8.0
Gozha et al.	2012	102.6	7.25	–	–	–	–
Piskunov et al.	2008	102.589	7.251	–	–	–	–
Kharchenko et al.	2007	102.6	7.25	–	0.17	–	8.0
Kharchenko et al.	2005	102.6	7.25	–	-3.05	-0.5	8.0
Dias et al.	2002	102.6	7.25	–	-0.73	-3.14	8.0

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	141	–	21	–	–
Kharchenko et al.	2016	0.98	0.40	–	141	–	–	–	–
Kharchenko et al.	2013	0.98	0.40	–	141	–	–	–	–
Gozha et al.	2012	0.80	–	–	123	–	29	–	–
Piskunov et al.	2008	0.80	0.40	–	123	–	–	–	–
Kharchenko et al.	2005	0.80	0.40	–	123	–	–	–	–
Dias et al.	2002	0.80	0.40	–	123	–	–	–	–

Visualization

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