NGC 6514

0.34 UTI

0.0

C_N

0.05

C_dens

0.5

C_C3

0.58

C_lit

1.0

C_dup

N_m (P>50%) 16

Core radius and density 2.6 [pc], 0.3 [pc^-2]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.58 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 6514 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.20 kpc) differs significantly from the median photometric distance (~0.82 kpc).

Close Low extinction Young

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: one or a few submm emission within the cluster area, but the submm emission is likely associated to the cluster.

Ahumada & Lapasset (2007)
Selected angular diameter from (1987, Lund Catalogue of Open Cluster Data).

Data

🔍 Search references for NGC 6514 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–	270.8	-22.945	0.313	-0.149	-1.7	-29.438
Jaehnig et al.	2021	270.656	-22.889	0.852	0.325	-1.699	–
Dib et al.	2018	270.645	-22.995	–	–	–	–
Loktin & Popova	2017	270.675	-22.973	–	3.1	-0.21	-2.1
Sampedro et al.	2017	270.675	-22.972	–	-0.83	-0.4	–
Joshi et al.	2016	270.645	-22.995	–	–	–	–
Dias et al.	2014	270.675	-22.972	–	-0.77	-0.7	–
Morales et al.	2013	270.675	-22.972	–	–	–	–
Gozha et al.	2012	270.675	-22.972	–	–	–	–
Piskunov et al.	2008	270.665	-22.973	–	–	–	–
Kharchenko et al.	2007	270.67	-22.97	–	0.23	–	-2.13
Ahumada & Lapasset	2007	270.675	-22.967	–	–	–	–
van den Bergh	2006	270.596	-23.03	–	–	–	–
Kharchenko et al.	2005	270.67	-22.97	–	2.63	-1.01	-2.13
Kharchenko et al.	2003	270.58	-23.02	–	0.63	-2.75	–
Chen et al.	2003	270.641	-23.053	–	-0.42	-3.02	-22.0
Dias et al.	2002	270.675	-22.972	–	-0.77	-0.7	-0.83
Dambis	1999	270.675	-22.972	–	–	–	–
Lynga	1987	270.588	-23.037	–	–	–	0.0
Sulentic et al.	1973	270.58	-23.032	–	–	–	–

💡 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–	0.82	0.6	–	20	–	138	–	0
Jaehnig et al.	2021	1.18⁽¹⁾	–	–	–	–	–	–	–
Dib et al.	2018	1.09	–	–	8	–	–	–	–
Loktin & Popova	2017	0.82	0.60	–	23	–	–	–	–
Joshi et al.	2016	1.09	1.05	–	8	–	138	–	–
Morales et al.	2013	2.70	–	–	–	–	–	–	–
Gozha et al.	2012	0.82	–	–	23	–	138	–	–
Piskunov et al.	2008	0.82	0.60	–	19	–	–	–	–
Ahumada & Lapasset	2007	–	0.60	–	23	–	–	–	0
van den Bergh	2006	0.82	0.60	–	23	–	–	–	–
Kharchenko et al.	2005	0.82	0.60	–	19	–	–	–	–
Kharchenko et al.	2003	0.82	0.60	–	–	–	–	–	–
Chen et al.	2003	0.82	–	–	20	–	–	–	–
Dias et al.	2002	0.82	0.60	–	23	–	–	–	–
Dambis	1999	0.83	0.68	–	8	–	–	–	–
Lynga	1987	1.60	0.91	–	–	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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