Taurus

0.38 UTI

0.25

C_N

0.92

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 25

Radius (P>50% members) 61.9 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.92 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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Taurus is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 4 later reported entries. See table with shared members information.

Low extinction Very young

Data

🔍 Search references for Taurus 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	–	65.782	27.292	7.718	8.8	-25.91	14.811
He et al.	2022	66.016	26.89	7.724	8.308	-24.137	–

💡 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
He et al.	2022	–	0.55	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 268	80.0	64.65	28.2	7.66	8.79	-25.31	14.92	0.39
HSC 1318	40.0	64.5	28.21	7.66	8.72	-25.42	15.41	0.0
Theia 7	12.0	68.63	24.72	7.68	6.71	-21.2	13.0	0.21
OCSN 52	4.0	68.73	24.35	7.74	7.0	-21.17	14.64	0.48

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

Visualization

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