2021PASJ...73.1486D


Query : 2021PASJ...73.1486D

2021PASJ...73.1486D - Publ. Astron. Soc. Jap., 73, 1486-1496 (2021/December-0)

Fundamental parameters for 30 faint open clusters with Gaia EDR3 based on the more reliable members.

DING X., JI K.-F., LI X.-Z., CHENG Q.-Y., WANG J.-L., YU X.-G. and LIU H.

Abstract (from CDS):

An open cluster is an ideal region to study the evolution of stars. In this work, we use Gaia Early Data Release 3 (Gaia EDR3) to derive the fundamental parameters of 30 faint open clusters listed in the catalogue given by Cantat-Gaudin et al. (2018, A&A, 618, A93), but the G magnitude of all of the member stars of that catalogue is brighter than ∼18 mag. This catalogue does not provide isochrone fitting parameters and spatial structure parameters. We acquired the member stars of 30 open clusters using the Density-Based Spatial Clustering of Applications with Noise algorithm in Gaia EDR3. The G magnitude of the member stars using our method can be found down to ∼21 mag. The G-band, GBP-band, and GRP-band data of the member stars construct a good color-magnitude diagram, which can further ensure the precision of isochrone fitting. We also calculated the spatial structure parameters, which are the core radius and the limiting radius, using Markov chain Monte Carlo algorithm.

Abstract Copyright: © The Author(s) 2021. Published by Oxford University Press on behalf of the Astronomical Society of Japan.

Journal keyword(s): methods: data analysis - methods: statistical - open clusters and associations: general

Simbad objects: 31

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Number of rows : 31
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Cl Berkeley 2 OpC 00 25 16.4 +60 23 33           ~ 37 0
2 NGC 136 OpC 00 31 35.1 +61 30 27           ~ 43 0
3 NGC 609 OpC 01 36 25.2 +64 32 23   12.31 11.0     ~ 32 0
4 NGC 1193 OpC 03 05 56.4 +44 22 58     12.6     ~ 97 0
5 Cl Berkeley 14 OpC 04 59 44.5 +43 29 12           ~ 52 1
6 NGC 1798 OpC 05 11 39.3 +47 41 28           ~ 85 0
7 Cl King 22 OpC 05 22 09.7 +45 26 30           ~ 81 0
8 DSH J0541.3+3914 OpC 05 41 25.3 +39 14 18           ~ 24 0
9 NGC 2112 OpC 05 53 47.5 +00 24 18     9.1     ~ 109 0
10 NGC 2158 OpC 06 07 26.7 +24 05 53           ~ 317 0
11 Cl Berkeley 23 OpC 06 33 15.6 +20 32 09           ~ 41 0
12 Cl Berkeley 24 OpC 06 37 48.0 -00 52 27           ~ 31 0
13 Cl Berkeley 27 OpC 06 51 20.9 +05 46 16           ~ 24 0
14 Cl Berkeley 31 OpC 06 57 37.5 +08 17 18           ~ 142 0
15 Cl Berkeley 30 OpC 06 57 45.1 +03 13 44           ~ 57 0
16 Cl Berkeley 33 OpC 06 57 49.7 -13 13 38           ~ 95 0
17 Cl Berkeley 34 OpC 07 00 22.7 -00 14 28           ~ 28 0
18 NGC 2324 OpC 07 04 08.5 +01 02 50   8.83 8.4     ~ 174 0
19 NAME Auner 1 OpC 07 04 14.4 -19 45 01           ~ 30 0
20 Cl Berkeley 35 OpC 07 09 57.2 +02 43 59           ~ 28 0
21 Cl Berkeley 78 OpC 07 23 38.3 +05 22 08           ~ 29 0
22 Cl Czernik 30 OpC 07 31 11.1 -09 56 47           ~ 50 0
23 NGC 2414 OpC 07 33 10.7 -15 26 56   8.33 7.9     ~ 87 0
24 Cl VDBH 19 OpC 08 07 04.3 -32 21 20           ~ 20 0
25 Cl VDBH 67 OpC 09 26 43.8 -51 16 22           ~ 19 0
26 Cl VDBH 73 OpC 09 31 55.0 -50 13 29           ~ 17 0
27 Cl VDBH 85 OpC 10 01 52.1 -49 33 50           ~ 22 0
28 NGC 3255 OpC 10 26 32.4 -60 40 30   11.54 11.0     ~ 36 0
29 Cl VDBH 118 OpC 11 23 02.3 -58 33 02           ~ 22 0
30 NGC 6791 OpC 19 20 52.8 +37 46 40   10.52 9.5     ~ 1120 0
31 Cl Berkeley 99 OpC 23 21 03.8 +71 46 44           ~ 41 0

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