FSR 1029

(MWSC 1012)

0.25 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.44

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 16

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.38 Low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 1029 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above 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 (~7.50 kpc) differs significantly from the median photometric distance (~1.91 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for FSR 1029 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	–	103.566	6.789	0.133	-0.342	-0.749	58.791
Just et al.	2023	103.508	6.727	–	–	–	–
Bica et al.	2019	103.524	6.726	–	–	–	–
Kharchenko et al.	2016	103.508	6.727	–	–	–	–
Dias et al.	2014	103.517	6.728	–	0.37	-7.96	–
Kharchenko et al.	2013	103.515	6.725	–	0.78	-3.98	–
Froebrich et al.	2007	103.517	6.728	–	–	–	–
Dias et al.	2002	103.517	6.728	–	0.27	-8.05	–

💡 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	–	–	–	851	–	155	–	–
Kharchenko et al.	2016	1.91	0.97	–	851	–	–	–	–
Kharchenko et al.	2013	1.91	0.97	–	851	–	–	–	–
Dias et al.	2002	1.91	0.97	–	851	–	–	–	–

Visualization

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