English

CCD Photometry of the Globular Cluster NGC 5897

Solar and Stellar Astrophysics 2023-11-14 v1

Abstract

We report CCD photometric observations of the globular cluster NGC 5897, in the Johnson system filters B, V , R, and I. With the values for these magnitudes we obtain various colour indices and produce several colour-magnitude diagrams. We present eight colour-magnitude diagrams: V vs B-V , B vs B-V , V vs V-I, I vs V-I, R vs R-I, I vs R-I, V vs V-R, and R vs V-R. In all of these diagrams we can clearly see the Giant Branch, the Horizontal Branch and the beginning of the Main Sequence. To the left of the Main Sequence turn-off point we detect a somewhat large number of Blue Straggler stars. We determine the mean value of the visual magnitude of the HB as 16.60±0.4616.60 \pm 0.46. This value is fainter than the value found by other authors.

Keywords

Cite

@article{arxiv.2311.07525,
  title  = {CCD Photometry of the Globular Cluster NGC 5897},
  author = {A. Ruelas-Mayorga and L. J. Sánchez and E. Macías-Estrada and A. Nigoche-Netro},
  journal= {arXiv preprint arXiv:2311.07525},
  year   = {2023}
}

Comments

28 pages, 7 figures, accepted for publication RevMexAA, vol. 60-1, April 2024. arXiv admin note: text overlap with arXiv:1606.04526