bdAbstract
The open cluster NGC 2818 containing a planetary nebula has been observed inVRI bands using the CCD system at prime focus of the 2.3-metre Vainu Bappu Telescope. The study extending to starsV ∼ 21 magnitude establishes the distance modulus as(m-M) 0 = 12.9 ±0.1 for the cluster. Based on the fitting of theoretical isochrones computed for solar metallicity, an age of 5(±1) × 108 years has been assigned to the cluster. Association of the planetary nebula with the cluster indicates that the progenitor mass of the planetary nebula on the main sequence is ≥2.5M⊙
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Based on observations obtained with the Vainu Bappu Telescope.
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Surendiranath, R., Rao, N.K., Sagar, R. et al. CCD photometry inVRI bands of the galactic cluster NGC 2818. J. Astrophys. Astr. 11, 151–166 (1990). https://doi.org/10.1007/BF02715014
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DOI: https://doi.org/10.1007/BF02715014