Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts [Data Set]
We provide the tabular data underlying the cooling curves plotted in Figures 6, 7, and 8 in the article "Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts" (accepted for publication in A&A, arXiv: 2608.03732) Each file corresponds to a single cooling curve. The first column is the decimal logarithm of age in seconds, and the second column is the decimal logarithm of redshifted surface photon luminosity in ergs per second. See the article for more details.
Authors
- Mikhail V. Beznogov (ORCID: https://orcid.org/0000-0002-7326-7270)
- Sagnik Chatterjee (ORCID: https://orcid.org/0000-0001-6367-7017)
- Ad. R. Raduta (ORCID: https://orcid.org/0000-0001-8421-2040)
- Dany Page
Institutions
- Horia Hulubei National Institute for R and D in Physics and Nuclear Engineering (RO)
- Universidad Nacional Autónoma de México (MX)
Publication Details
- Journal
- arXiv (Cornell University)
- Published
- 2026-10-13
- DOI
- https://doi.org/10.5281/zenodo.23343163
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- preprint
Funders
- Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii
- Colegiul Consultativ pentru Cercetare-Dezvoltare şi Inovare