Photometric survey of marginally investigated open clusters I. Basel 11b, King 14, Czernik 43

被引:3
|
作者
Netopil, M
Maitzen, HM
Paunzen, E
Claret, A
机构
[1] Univ Vienna, Inst Astron, A-1180 Vienna, Austria
[2] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
关键词
techniques : photometric; Galaxy : open clusters and associations : general;
D O I
10.1051/0004-6361:20054707
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. To progress in galactic studies based on open clusters, e. g. cluster formation rate or kinematical properties, one needs to improve the number of open clusters observed. However, only half of the 1700 known galactic open clusters have been properly observed so far, making any statistical investigation insignificant, especially at larger distances from the Sun. Methods. We study marginally investigated or neglected open clusters with Bessell CCD BVR photometry, whose data were used to fit isochrones to the individual color-magnitude diagrams. Results. We examined the galactic clusters Basel 11b, King 14 and Czernik 43, the last being observed for the first time to this extent. As well as a careful comparison to available photometry, their parameters such as age, interstellar reddening, distance and apparent diameter were determined. The obtained cluster properties were verified by near infrared 2MASS data. The three investigated intermediate age clusters are all located in the galactic disk with distances between 1.8 and 3.0 kpc from the Sun.
引用
收藏
页码:179 / 184
页数:6
相关论文
共 5 条
  • [1] Photometric survey of marginally investigated open clusters I. Basel 11b, King 14, Czernik 43
    Netopil, M.
    Maitzen, H.M.
    Paunzen, E.
    Claret, A.
    Astronomy and Astrophysics, 1600, 454 (01): : 179 - 184
  • [2] Photometric monitoring of open clusters. I. The survey
    Hebb, L
    Wyse, RFG
    Gilmore, G
    ASTRONOMICAL JOURNAL, 2004, 128 (06): : 2881 - 2897
  • [3] The OPD photometric survey of open clusters I. Techniques, program details and first results of robust determination of the fundamental parameters
    Caetano, T. C.
    Dias, W. S.
    Lepine, J. R. D.
    Monteiro, H. S.
    Moitinho, A.
    Hickel, G. R.
    Oliveira, A. F.
    NEW ASTRONOMY, 2015, 38 : 31 - 49
  • [4] Cluster Difference Imaging Photometric Survey. I. Light Curves of Stars in Open Clusters from TESS Sectors 6 and 7
    Bouma, L. G.
    Hartman, J. D.
    Bhatti, W.
    Winn, J. N.
    Bakos, G. A.
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2019, 245 (01):
  • [5] Production cross sections of fragments from beams of 400-650 MeV per nucleon 9Be, 11B, 12C, 14N, 15N, 16O, 20Ne, 22Ne, 56Fe, and 58Ni nuclei interacting in a liquid hydrogen target.: I.: Charge changing and total cross sections
    Webber, WR
    Kish, JC
    Rockstroh, JM
    Cassagnou, Y
    Legrain, R
    Soutoul, A
    Testard, O
    Tull, C
    ASTROPHYSICAL JOURNAL, 1998, 508 (02): : 940 - 948