Erratum: Magnetars: super(ficially) hot and super(fluid) cool
Article first published online: 22 AUG 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 425, Issue 2, page 1600, 11 September 2012
How to Cite
Ho, W. C. G., Glampedakis, K. and Andersson, N. (2012), Erratum: Magnetars: super(ficially) hot and super(fluid) cool. Monthly Notices of the Royal Astronomical Society, 425: 1600. doi: 10.1111/j.1365-2966.2012.21441.x
- Issue published online: 22 AUG 2012
- Article first published online: 22 AUG 2012
Vol. 422, Issue 3, 2632–2641, Article first published online: 4 APR 2012
- errata, addenda;
- dense matter;
- stars: evolution;
- stars: magnetars;
- stars: neutron;
- pulsars: general
The paper ‘Magnetars: super(ficially) hot and super(fluid) cool’ was published in Mon. Not. R. Astron. Soc. 422, 2632–2641 (2012). An error in the original work of van Riper (1991) was reproduced in our paper. Equations (10) and (11) for the ion heat capacity should read
In equation (10), the expression for Cion in the range 1 < Γc ≤ 150 is simply a smooth interpolation between the expressions in the range Γc ≤ 1 and Γc > 150. In equation (11), the value of 0.4 for the range is needed in order for fD(T/TD) to be smooth.
The remainder of the paper remains unaffected by these corrections since the primary effect of the ion heat capacity is on the thermal relaxation time of the crust, which is not the concern of our paper. We note that we have subsequently implemented more accurate ion and electron heat capacities from Potekhin & Chabrier (2010).
We thank José Pons for pointing out these errors.