Markarian 6

0.48 UTI

0.0

C_N

1.0

C_dens

0.75

C_C3

0.31

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 24

Radius (P>50% members) 3.2 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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Markarian 6 is a sparse, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 9 years.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Close Moderate extinction Low mass Very young

Data

🔍 Search references for Markarian 6 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	–	37.429	60.685	1.467	-3.548	0.482	-5.885
Loktin & Popova	2017	37.41	60.707	–	-1.343	-2.513	-7.18
Dias et al.	2014	37.417	60.707	–	-4.44	0.32	–
Gozha et al.	2012	37.417	60.707	–	–	–	–
Kharchenko et al.	2003	37.41	60.67	–	-4.8	-1.73	–
Dias et al.	2002	37.417	60.707	–	-3.33	0.24	-7.18

💡 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
Loktin & Popova	2017	0.59	1.71	–	16	–	–	–	–
Gozha et al.	2012	0.70	–	–	16	–	30	–	–
Kharchenko et al.	2003	0.70	1.77	–	–	–	–	–	–
Dias et al.	2002	0.70	1.88	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 7	100.0	37.44	60.61	1.47	-3.53	0.46	-7.82	0.8

💡 Note: The % column shows the percentage of members that Markarian 6 shares with each listed object.

Visualization

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