2007PASP..119.1093J


Query : 2007PASP..119.1093J

2007PASP..119.1093J - Publ. Astron. Soc. Pac., 119, 1093-1098 (2007/October-0)

The consistency of Stromgren-β photometry for northern galactic clusters. IV. Praesepe revisited and the Pleiades.

JONER M.D. and TAYLOR B.J.

Abstract (from CDS):

New Strömgren-β Pleiades data on a zero point defined by the Hyades and Coma are presented. The new data and counterparts from four extant sources are compared to measurements published by Crawford & Perry in 1976. The only statistically significant problem found in this way is a 4 mmag b-y offset obtained from a data set published by McNamara in 1976.
Result. of similar comparisons published previously for Praesepe are updated by including three additional sets of published data. In this case, comparisons are made to measurements published by Crawford & Barnes in 1969. Two of the data sets (including one published by Joner & Taylor in 1995) yield accordant, statistically significant formal corrections to the b-y, m1, and β measurements of Crawford & Barnes. In addition, results from a third data set are consistent with those derived from the data of Joner & Taylor. However, this pattern is either partly or entirely absent from the offsets yielded by the other three data sets. Because the measurements of Joner & Taylor are still the only ones known to have been derived from direct comparisons among the Hyades, Coma, and Praesepe, it is concluded that the balance of evidence presently favors the offsets obtained from those data. In addition, it is noted that the data of Joner & Taylor do not imply that the data of Crawford & Barnes require corrections that depend on color. With these interim conclusions drawn, it is then suggested that further Praesepe measurements should be brought to bear on the problem.

Abstract Copyright: ∼

Journal keyword(s): Star Clusters and Associations

Simbad objects: 24

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Number of rows : 24
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 NGC 752 OpC 01 56 53.7 +37 45 06           ~ 712 0
2 HD 23157 ** 03 43 41.5325750160 +23 38 56.977320660   8.25 7.95     A5V 99 0
3 HD 23158 SB* 03 43 42.8773509420 +23 35 41.208537362   10.04 9.58     F5V 88 0
4 V* V1187 Tau dS* 03 44 00.2690335032 +24 33 25.193571588   8.28 8.07     A4IV 156 0
5 HD 23247 PM* 03 44 23.5411594200 +24 07 57.471196908   9.564 9.111 9.23   F2V 95 0
6 * 16 Tau V* 03 44 48.2149362048 +24 17 22.083331452 5.09 5.42 5.46 5.42 5.47 B7V 272 0
7 * 18 Tau PM* 03 45 09.7401340368 +24 50 21.343198416 5.21 5.57 5.64 5.61 5.68 B8V 293 0
8 HD 23409 * 03 45 51.6357297648 +24 02 19.955007204   8.11 7.92   7.63 A2V 101 0
9 * 21 Tau PM* 03 45 54.4764507648 +24 33 16.235698248 5.49 5.72 5.76 5.71 5.74 B8V 234 0
10 * 22 Tau ** 03 46 02.9003257344 +24 31 40.428415632   6.402 6.421   6.41 A0Vn 183 0
11 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0
12 HD 23511 PM* 03 46 39.3335012425 +24 06 11.531508492   9.75 9.28   8.75 F5V 144 0
13 HD 23513 PM* 03 46 39.9969863424 +23 06 37.194884441 9.85 9.91 9.40 8.97 8.83 F5V 115 0
14 HD 23584 * 03 47 10.0537991349 +24 16 35.945010583   9.99 9.58   8.92 F6V 102 0
15 * 24 Tau * 03 47 21.0386292336 +24 06 58.564163952 6.26 6.30 6.28   6.30 A0V 105 0
16 HD 23753 PM* 03 48 20.8167826752 +23 25 16.495877028 5.06 5.38 5.45 5.42 5.48 B8V 194 0
17 HD 23872 * 03 49 16.8025399608 +24 23 46.065811884   7.64 7.54   7.34 A2V 97 0
18 HD 23923 * 03 49 43.5315887616 +23 42 42.667696476   6.104 6.153   6.18 B8.5V 173 0
19 HD 23948 * 03 49 56.5953892752 +24 20 56.372246016   7.61 7.54   7.48 A0 108 0
20 HD 24132 * 03 51 27.2143557432 +24 31 07.142738880 9.3 9.24 8.84 8.49 8.40 F2Vn 103 0
21 Cl Melotte 25 OpC 04 30 27.4 +16 46 43           ~ 3309 0
22 NGC 2632 OpC 08 39 58.4 +19 36 33           ~ 1733 0
23 NGC 2682 OpC 08 51 23.5 +11 48 54           ~ 2528 0
24 Cl Melotte 111 OpC 12 11 54.9 +25 16 36           ~ 520 0

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