The crucial discovery of thermonuclear X-ray bursts: never throw away old data!
Fuente:
arXiv
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| Autore principale: | |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| Accesso online: | |
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| _version_ | 1866912107375624192 |
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| author | Kuulkers, Erik |
| author_facet | Kuulkers, Erik |
| contents | The detection of Type I X-ray bursts is attributed to those seen by the Astronomical Netherlands Satellite (ANS) in September 1975 from the globular cluster NGC6624 containing the X-ray source 4U1820-303. I revisit these X-ray bursts, by re-analysing data from the Soft X-ray Experiment (SXX) onboard ANS, which were stored on microfiche. Earlier accounts of X-ray bursts had been reported; the first Type I X-ray burst recorded is the one observed by Vela 5B from Cen X-4 in July 1969. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_03911 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The crucial discovery of thermonuclear X-ray bursts: never throw away old data! Kuulkers, Erik High Energy Astrophysical Phenomena Solar and Stellar Astrophysics The detection of Type I X-ray bursts is attributed to those seen by the Astronomical Netherlands Satellite (ANS) in September 1975 from the globular cluster NGC6624 containing the X-ray source 4U1820-303. I revisit these X-ray bursts, by re-analysing data from the Soft X-ray Experiment (SXX) onboard ANS, which were stored on microfiche. Earlier accounts of X-ray bursts had been reported; the first Type I X-ray burst recorded is the one observed by Vela 5B from Cen X-4 in July 1969. |
| title | The crucial discovery of thermonuclear X-ray bursts: never throw away old data! |
| topic | High Energy Astrophysical Phenomena Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2411.03911 |