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Can the anomalous X-ray pulsar 4U 0142+61 be described as an accreting white dwarf?
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On the Electromagnetic Emission of SGRs/AXPs as White Dwarf and Neutron Star Pulsars
| MG15 | Rome 1 - 7 July, 2018 | University Map |
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Session: |
WD2 - Origin and physics of Soft Gamma-ray Repeaters and Anomalous X-ray Pulsars |
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Chairperson: |
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Day: |
Friday, July 6 |
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Room: |
ChC - AULA C - CU014 |
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| Arrived | Accept | N. | Hour | Time | Talk Type | Speaker | Talk Title | Talk view |
| √ | Yes |
1 |
15:15 | 25' + 5' | Oral abstract | |||
| √ | Yes |
2 |
15:45 | 25' + 5' | Oral abstract | |||
| √ | Yes |
3 |
16:15 | 25' + 5' | Oral abstract |
Can the anomalous X-ray pulsar 4U 0142+61 be described as an accreting white dwarf? |
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| √ | Yes |
4 |
17:15 | 25' + 5' | Oral abstract | |||
| √ | Yes |
5 |
17:45 | 15' + 5' | Oral abstract | |
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| √ | Yes |
6 |
18:05 | 15' + 5' | Oral abstract |
On the Electromagnetic Emission of SGRs/AXPs as White Dwarf and Neutron Star Pulsars |
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