The population of faint transients in the galactic centre
BeppoSAX has detected a population of faint transient Xray sources in the Galactic Centre. I show that a simple irradiated-disc picture gives a consistent fit to the properties of this population, and that it probably consists of low-mass X-ray binaries which have evolved beyond their minimum orbita...
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2001
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| _version_ | 1826268677580783616 |
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| author | King, A |
| author_facet | King, A |
| author_sort | King, A |
| collection | OXFORD |
| description | BeppoSAX has detected a population of faint transient Xray sources in the Galactic Centre. I show that a simple irradiated-disc picture gives a consistent fit to the properties of this population, and that it probably consists of low-mass X-ray binaries which have evolved beyond their minimum orbital periods similar to 80 min. Since all post-minimum systems are transient, and neutron-star LMXBs are more common than black-hole LMXBs in the Galaxy, the majority of these systems should contain neutron stars, as observed. This picture predicts that the Galactic Centre transients should have orbital periods in the range similar to 80-120 minutes, and that most of them should repeat in the next few years. In this case, the total number of post-minimum transients in the Galaxy would be considerably smaller than the usual estimates of its total LMXB population. I discuss possible reasons for this. |
| first_indexed | 2024-03-06T21:13:22Z |
| format | Conference item |
| id | oxford-uuid:3eee4f1c-253c-4f2a-a3f1-23445e783656 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T21:13:22Z |
| publishDate | 2001 |
| record_format | dspace |
| spelling | oxford-uuid:3eee4f1c-253c-4f2a-a3f1-23445e7836562022-03-26T14:28:46ZThe population of faint transients in the galactic centreConference itemhttp://purl.org/coar/resource_type/c_5794uuid:3eee4f1c-253c-4f2a-a3f1-23445e783656Symplectic Elements at Oxford2001King, ABeppoSAX has detected a population of faint transient Xray sources in the Galactic Centre. I show that a simple irradiated-disc picture gives a consistent fit to the properties of this population, and that it probably consists of low-mass X-ray binaries which have evolved beyond their minimum orbital periods similar to 80 min. Since all post-minimum systems are transient, and neutron-star LMXBs are more common than black-hole LMXBs in the Galaxy, the majority of these systems should contain neutron stars, as observed. This picture predicts that the Galactic Centre transients should have orbital periods in the range similar to 80-120 minutes, and that most of them should repeat in the next few years. In this case, the total number of post-minimum transients in the Galaxy would be considerably smaller than the usual estimates of its total LMXB population. I discuss possible reasons for this. |
| spellingShingle | King, A The population of faint transients in the galactic centre |
| title | The population of faint transients in the galactic centre |
| title_full | The population of faint transients in the galactic centre |
| title_fullStr | The population of faint transients in the galactic centre |
| title_full_unstemmed | The population of faint transients in the galactic centre |
| title_short | The population of faint transients in the galactic centre |
| title_sort | population of faint transients in the galactic centre |
| work_keys_str_mv | AT kinga thepopulationoffainttransientsinthegalacticcentre AT kinga populationoffainttransientsinthegalacticcentre |