The CCD Photometry of the Globular Cluster NGC 362

Details The CCD Photometry of the Globular Cluster NGC 362 The CCD Photometry of the Globular Cluster NGC 362

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jkas...31...19l&link_type=abstract

Journal of the Korean Astronomical Society, vol. 31, No. 1, pp. 19-26

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Globular Cluster, C-M Diagram, Luminosity Function, Theoretical Isochrone

Scientific paper

The wide field (~ 20' X 20') CCD photometry has been performed for more than 4,000 stars over a whole region of NGC 362 which is located inside the SMC halo. The Color-Magnitude diagram (CMD) and luminosit function (LF) for red giant branch (RGB) stars are presented, discussing a distinct bump along the RGB and some blue stars appearing in the blue horizontal branch (BHB) and above BHB. The anomalous globular cluster NGC 362 with highly populated red horizontal branch (RHB) stars is compared with the another anomalous globular cluster NGC 288 with highly populated BHB stars. A metal-rich, young blue component and metal-poor, old red component of the SMC halo stars are examined.

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