Free Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201118287]


Issue
A&A
Volume 541, May 2012
Article Number C3
Number of page(s) 1
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201118287e
Published online 24 May 2012

It has been pointed out to the author that in Sect. 6 of this paper, an incorrect mass was used to calculate the predicted mass loss for the cluster NGC 6791. The mass used of 1.6 M referred to the other cluster discussed in Miglio et al. (2012), NGC 6819.

Although the values given in Table 6 of the paper are correct, the inferences drawn from them need to be modified, even though all conclusions remain unchanged.

Table 1 lists the predicted mass loss for an initial mass of 1.2 M (Miglio et al. determined the mass of stars on the RGB of NGC 6719 to be about 1.23 M).

As the mass loss for a lower initial mass is larger on the RGB, the scaling factors η1 and η2 are lower, namely η1 = 7.5    ±    4 and η2 = 9    ±    5.

The factor mentioned in the sentence of the abstract “Using a scaling factor of  ~ 10    ±     ~ 5, both relations can fit this value”. should be  ~ 8    ±     ~ 5.

Table 1

Mass lost on the RGB for a 1.2 M star.

Acknowledgments

MG would like to thank Dr. Andrea Miglio for pointing out this mistake.

References

  1. Miglio, A., Brogaard, K., Stello, D., et al. 2012, MNRAS, 419, 2077 [NASA ADS] [CrossRef] [Google Scholar]

© ESO, 2012

All Tables

Table 1

Mass lost on the RGB for a 1.2 M star.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.