Erratum: ``Planetary Nebulae in the Globular Clusters PAL 6 and NGC 6441'' [Astron. J. 114, 2611 (1997)]

Astronomy and Astrophysics – Astronomy

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The conclusion on page 2623 was incorrectly printed; it should read as follows: (5) If, in fact, a low mass single star (e.g., the 0.8 M_&sun; stars in GCs) cannot form a PN, then, contrary to common belief, it becomes questionable whether a single 1 M_&sun; star (e.g., the Sun) will go through a PN phase. The uncertainty in the initial-to-final mass relation at low masses is sufficiently large that the future evolutionary path of the Sun may need to be reevaluated.

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