Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058
We present quasi-simultaneous radio (VLA) and X-ray (Swift) observations of the neutron star low-mass X-ray binary (NS-LMXB) 1RXS J180408.9-342058 (J1804) during its 2015 outburst. We found that the radio jet of J1804 was bright (232 ± 4 µJy at 10 GHz) during the initial hard X-ray state, before bei...
| Main Authors: | , , , , , , , , |
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| Format: | Journal Article |
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Oxford University Press
2017
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| Online Access: | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/55610 |
| _version_ | 1848759664170237952 |
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| author | Gusinskaia, N. Deller, A. Hessels, J. Degenaar, N. Miller-Jones, James Wijnands, R. Parikh, A. Russell, T. Altamirano, D. |
| author_facet | Gusinskaia, N. Deller, A. Hessels, J. Degenaar, N. Miller-Jones, James Wijnands, R. Parikh, A. Russell, T. Altamirano, D. |
| author_sort | Gusinskaia, N. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | We present quasi-simultaneous radio (VLA) and X-ray (Swift) observations of the neutron star low-mass X-ray binary (NS-LMXB) 1RXS J180408.9-342058 (J1804) during its 2015 outburst. We found that the radio jet of J1804 was bright (232 ± 4 µJy at 10 GHz) during the initial hard X-ray state, before being quenched by more than an order of magnitude during the soft X-ray state (19 ± 4 µJy). The source then was undetected in radio ( < 13 µJy) as it faded to quiescence. In NS-LMXBs, possible jet quenching has been observed in only three sources and the J1804 jet quenching we show here is the deepest and clearest example to date. Radio observations when the source was fading towards quiescence (L X = 10 34-35 erg s -1 ) show that J1804 must follow a steep track in the radio/X-ray luminosity plane with ß > 0.7 (where L R a L X ß ). Few other sources have been studied in this faint regime, but a steep track is inconsistent with the suggested behaviour for the recently identified class of transitional millisecond pulsars. J1804 also shows fainter radio emission at L X < 10 35 erg s -1 than what is typically observed for accreting millisecond pulsars. This suggests that J1804 is likely not an accreting X-ray or transitional millisecond pulsar. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. |
| first_indexed | 2025-11-14T10:03:28Z |
| format | Journal Article |
| id | curtin-20.500.11937-55610 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T10:03:28Z |
| publishDate | 2017 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-556102022-11-28T04:13:44Z Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 Gusinskaia, N. Deller, A. Hessels, J. Degenaar, N. Miller-Jones, James Wijnands, R. Parikh, A. Russell, T. Altamirano, D. We present quasi-simultaneous radio (VLA) and X-ray (Swift) observations of the neutron star low-mass X-ray binary (NS-LMXB) 1RXS J180408.9-342058 (J1804) during its 2015 outburst. We found that the radio jet of J1804 was bright (232 ± 4 µJy at 10 GHz) during the initial hard X-ray state, before being quenched by more than an order of magnitude during the soft X-ray state (19 ± 4 µJy). The source then was undetected in radio ( < 13 µJy) as it faded to quiescence. In NS-LMXBs, possible jet quenching has been observed in only three sources and the J1804 jet quenching we show here is the deepest and clearest example to date. Radio observations when the source was fading towards quiescence (L X = 10 34-35 erg s -1 ) show that J1804 must follow a steep track in the radio/X-ray luminosity plane with ß > 0.7 (where L R a L X ß ). Few other sources have been studied in this faint regime, but a steep track is inconsistent with the suggested behaviour for the recently identified class of transitional millisecond pulsars. J1804 also shows fainter radio emission at L X < 10 35 erg s -1 than what is typically observed for accreting millisecond pulsars. This suggests that J1804 is likely not an accreting X-ray or transitional millisecond pulsar. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. 2017 Journal Article http://hdl.handle.net/20.500.11937/55610 10.1093/mnras/stx1235 http://purl.org/au-research/grants/arc/FT140101082 Oxford University Press fulltext |
| spellingShingle | Gusinskaia, N. Deller, A. Hessels, J. Degenaar, N. Miller-Jones, James Wijnands, R. Parikh, A. Russell, T. Altamirano, D. Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title | Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title_full | Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title_fullStr | Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title_full_unstemmed | Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title_short | Jet quenching in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 |
| title_sort | jet quenching in the neutron star low-mass x-ray binary 1rxs j180408.9-342058 |
| url | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/55610 |