The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing
We present an analysis of 23 yr of pulse arrival times for PSR B1259−63. The pulsar is in a binary orbit about its approximately 20 M⊙ companion LS 2883. Our best-fitting timing solution has none of the pulse-number ambiguities that have plagued previous attempts to model the binary orbit. We measur...
| Main Authors: | , , |
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| Format: | Journal Article |
| Published: |
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/14567 |
| _version_ | 1848748657387503616 |
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| author | Shannon, Ryan Johnston, S. Manchester, R. |
| author_facet | Shannon, Ryan Johnston, S. Manchester, R. |
| author_sort | Shannon, Ryan |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | We present an analysis of 23 yr of pulse arrival times for PSR B1259−63. The pulsar is in a binary orbit about its approximately 20 M⊙ companion LS 2883. Our best-fitting timing solution has none of the pulse-number ambiguities that have plagued previous attempts to model the binary orbit. We measure significant first and second time derivatives of the projected semimajor axis and longitude of the periastron of the orbit. These variations are found to be consistent with the precession of the orbital plane due to classical spin–orbit coupling. The derived moment of inertia and spin of the companion are consistent with the companion rotating at near-break-up velocity. The system configuration is also consistent with the geometry derived from both the polarization of the radio emission and the eclipse of the pulsar by the equatorial disc of the companion. We find strong evidence for orbital period decay that can be attributed to mass-loss from the companion star. We also measure a significant proper motion that locates the birth of the system in the Centaurus OB1 association. By combining proper motion of the pulsar with radial velocity measurements of the companion, we measure the three-dimensional velocity of the system. This velocity is used to constrain the masses of the stars prior to the supernova explosion and the kick the pulsar received at or immediately after the explosion. |
| first_indexed | 2025-11-14T07:08:31Z |
| format | Journal Article |
| id | curtin-20.500.11937-14567 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T07:08:31Z |
| publishDate | 2014 |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-145672017-09-13T15:02:45Z The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing Shannon, Ryan Johnston, S. Manchester, R. We present an analysis of 23 yr of pulse arrival times for PSR B1259−63. The pulsar is in a binary orbit about its approximately 20 M⊙ companion LS 2883. Our best-fitting timing solution has none of the pulse-number ambiguities that have plagued previous attempts to model the binary orbit. We measure significant first and second time derivatives of the projected semimajor axis and longitude of the periastron of the orbit. These variations are found to be consistent with the precession of the orbital plane due to classical spin–orbit coupling. The derived moment of inertia and spin of the companion are consistent with the companion rotating at near-break-up velocity. The system configuration is also consistent with the geometry derived from both the polarization of the radio emission and the eclipse of the pulsar by the equatorial disc of the companion. We find strong evidence for orbital period decay that can be attributed to mass-loss from the companion star. We also measure a significant proper motion that locates the birth of the system in the Centaurus OB1 association. By combining proper motion of the pulsar with radial velocity measurements of the companion, we measure the three-dimensional velocity of the system. This velocity is used to constrain the masses of the stars prior to the supernova explosion and the kick the pulsar received at or immediately after the explosion. 2014 Journal Article http://hdl.handle.net/20.500.11937/14567 10.1093/mnras/stt2123 unknown |
| spellingShingle | Shannon, Ryan Johnston, S. Manchester, R. The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title | The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title_full | The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title_fullStr | The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title_full_unstemmed | The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title_short | The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing |
| title_sort | kinematics and orbital dynamics of the psr b1259-63/ls 2883 system from 23 yr of pulsar timing |
| url | http://hdl.handle.net/20.500.11937/14567 |