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- W4299573887 abstract "We have monitored the quasi-persistent neutron-star X-ray transient MXB 1659-29 in quiescence using Chandra. The purpose of our observations was to monitor the quiescent behavior of the source after its last prolonged outburst episode and to study the cooling curve of the neutron star in this system. We discuss the results obtained and how they constrain the properties of the neutron star in MXB 1659-29" @default.
- W4299573887 created "2022-10-02" @default.
- W4299573887 creator A5087214327 @default.
- W4299573887 date "2004-03-04" @default.
- W4299573887 modified "2023-10-18" @default.
- W4299573887 title "The crust cooling curve of the neutron star in MXB 1659-29" @default.
- W4299573887 doi "https://doi.org/10.48550/arxiv.astro-ph/0403117" @default.
- W4299573887 hasPublicationYear "2004" @default.
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