# Thermonuclear burst observations for model comparisons: a reference   sample

**Authors:** Duncan K. Galloway (1, 2), Adelle J. Goodwin (1), Laurens Keek (3, and 4) ((1) School of Physics, Astronomy, Monash University, (2) Monash, Centre for Astrophysics, (3) X-ray Astrophysics Laboratory, Astrophysics, Science Division, NASA/GSFC, (4) CRESST, the Department of Astronomy,, University of Maryland)

arXiv: 1703.07485 · 2017-04-26

## TL;DR

This paper compiles and analyzes observations of various thermonuclear X-ray bursts, providing detailed data sets to serve as benchmarks for testing and improving theoretical ignition models.

## Contribution

It presents a curated sample of burst observations with detailed properties, facilitating direct comparison with numerical ignition simulations and advancing understanding of burst mechanisms.

## Key findings

- Identification of four distinct ignition cases
- Measured recurrence times and burst profiles
- Provided data sets for model validation

## Abstract

We present a sample of observations of thermonuclear (type-I) X-ray bursts, selected for comparison with numerical models. Provided are examples of four distinct cases of thermonuclear ignition: He-ignition in mixed H/He fuel (case 1 of Fujimoto et al. 1981); He-ignition in pure He fuel, following exhaustion of accreted H by steady burning (case 2); ignition in (almost) pure He accumulated from an evolved donor in an ultracompact system; and an example of a superburst, thought to arise from ignition of a layer of carbon fuel produced as a by-product of more frequent bursts. For regular bursts, we measured the recurrence time and calculated averaged burst profiles from RXTE observations. We have also estimated the recurrence time for pairs of bursts, including those observed during a transient outburst modelled using a numerical ignition code. For each pair of bursts we list the burst properties including recurrence time, fluence and peak flux, the persistent flux level (and inferred accretion rate) as well as the ratio of persistent flux to fluence. In the accompanying material we provide a bolometric lightcurve for each burst, determined from time-resolved spectral analysis. Along with the inferred or adopted parameters for each burst system, including distance, surface gravity, and redshift, these data are suggested as a suitable test cases for ignition models.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1703.07485/full.md

## References

65 references — full list in the complete paper: https://tomesphere.com/paper/1703.07485/full.md

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Source: https://tomesphere.com/paper/1703.07485