2024PASP..136f4201M


Query : 2024PASP..136f4201M

2024PASP..136f4201M - Publ. Astron. Soc. Pac., 136, part no 6, 4201 (2024/June-0)

A Suite of Classical Cepheids Tied to the Binary Cluster Berkeley 58 and NGC 7790.

MAJAESS D. and TURNER D.G.

Abstract (from CDS):

The classical Cepheids CE Cas A, CE Cas B, CF Cas, and CG Cas are likely members of the binary open cluster comprising NGC 7790 and Berkeley 58. The clusters are of comparable age and in close proximity, as deduced from differentially dereddened UuBPBVGRP photometry, and Cepheid period-age relations. Gaia DR3 astrometric and spectroscopic solutions for the clusters are likewise consistent. Conversely, the seemingly adjacent open cluster NGC 7788 is substantially younger and nearer.

Abstract Copyright: © 2024. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved

Journal keyword(s): Star clusters - Cepheid variable stars

Simbad objects: 14

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Number of rows : 14
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 58 OpC 00 00 17.4 +60 56 28   10.39 9.7     ~ 72 0
2 V* CG Cas cC* 00 00 59.2385245512 +60 57 32.432852268   12.70 11.28     F5 113 0
3 Cl Blanco 1 OpC 00 03 04.1 -29 48 55           ~ 380 0
4 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0
5 Cl Melotte 25 OpC 04 30 27.4 +16 46 43           ~ 3309 0
6 NGC 2451 Cl* 07 45.4 -37 58           ~ 165 1
7 V* BB Sgr cC* 18 50 59.8729954248 -20 17 42.829838520 8.07 7.53 6.69   5.824 G0Ib 269 0
8 Cl Collinder 394 OpC 18 52 34.9 -20 10 39     6.3     ~ 96 0
9 NGC 6716 OpC 18 53 54.4 -19 57 44   7.70 7.5     ~ 85 0
10 NGC 7788 OpC 23 56 43.3 +61 23 54     9.4     ~ 78 0
11 V* CE Cas B cC* 23 58 09.1062438336 +61 12 49.078923084   12.27 11.20     F8Ib 52 0
12 V* CE Cas A cC* 23 58 09.4463569272 +61 12 49.336242768   12.15 10.95     F9Ib 59 0
13 V* CF Cas cC* 23 58 17.9760671064 +61 13 15.821693832   12.72 10.80   9.700 F8Ibv 256 0
14 NGC 7790 OpC 23 58 27.6 +61 12 33   9.18 8.5     ~ 286 0

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