FSR 1297

(MWSC 1207)

0.06 UTI

0.69

C_N

1.0

C_dens

0.62

C_C3

0.5

C_lit

0.09

C_dup

C3 classification AC

Number of members (P>50%) 88

Radius (P>50% members) 8.5 [arcmin]

C_N 0.69 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.5 Moderately studied
C_dup 0.09 Very likely duplicate

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

Overview

ℹ️

FSR 1297 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close^* distance, below the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is moderately studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~1.32 kpc) differs significantly from the median photometric distance (~2.46 kpc).

Relatively close Very high extinction Very young

Data

🔍 Search references for FSR 1297 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	110.982	-25.877	0.76	-2.705	3.282	38.556
Celli et al.	2024	110.984	-25.879	–	–	–	–
Just et al.	2023	110.987	-25.898	–	–	–	–
Cantat-Gaudin et al.	2020	110.984	-25.879	0.754	-2.775	3.314	–
Cantat-Gaudin & Anders	2020	110.984	-25.879	0.754	-2.775	3.314	–
Cantat-Gaudin et al.	2018	110.984	-25.879	0.754	-2.775	3.314	–
Kharchenko et al.	2016	110.987	-25.898	–	–	–	–
Kharchenko et al.	2013	110.992	-25.9	–	-1.56	2.55	–
Froebrich et al.	2007	111.0	-25.896	–	–	–	–

💡 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
Celli et al.	2024	–	–	–	5	–	148	–	–
Just et al.	2023	–	–	–	5	–	1227	–	–
Cantat-Gaudin & Anders	2020	1.28	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.28	–	–	–	–	–	–	–
Kharchenko et al.	2016	3.65	5.16	–	5	–	–	–	–
Kharchenko et al.	2013	3.65	5.16	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 88	90.9	110.98	-25.87	0.76	-2.67	3.28	38.55	0.59

💡 Note: The % column shows the percentage of members that FSR 1297 shares with each listed object.

Visualization

ℹ️

1 2