Sh2 235

(MWSC 629)

0.06 UTI

0.0

C_N

0.27

C_dens

0.62

C_C3

0.25

C_lit

0.2

C_dup

C3 classification AC

Number of members (P>50%) 19

Radius (P>50% members) 7.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.27 Loose
C_C3 0.62 Intermediate quality
C_lit 0.25 Poorly studied
C_dup 0.2 Likely duplicate

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

Overview

ℹ️

Sh2 235 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Very young

Data

🔍 Search references for Sh2 235 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	85.217	35.887	0.587	0.297	-2.972	–
Just et al.	2023	85.168	35.921	–	–	–	–
Kharchenko et al.	2016	85.168	35.921	–	–	–	–
Kharchenko et al.	2013	85.177	35.92	–	2.11	-3.43	–
Kharchenko et al.	2012	85.177	35.92	–	3.27	-3.93	–

💡 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	–	–	–	4	–	75	–	–
Kharchenko et al.	2016	2.31	3.23	–	4	–	–	–	–
Kharchenko et al.	2013	2.31	3.23	–	4	–	–	–	–
Kharchenko et al.	2012	1.10	1.24	–	1084	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0784	80.0	85.2	35.89	0.6	0.35	-2.97	-4.38	0.29
BDSB 73	40.0	85.36	35.86	0.59	0.46	-2.96	-4.38	0.17
FSR 0788	40.0	85.35	35.81	0.6	0.35	-2.83	–	0.3

💡 Note: The % column shows the percentage of members that Sh2 235 shares with each listed object.

Visualization

ℹ️