Strongly polarised radio pulses from a new white-dwarf-hosting long-period transient
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arXiv
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| Auteurs principaux: | , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866913930056564736 |
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| author | Bloot, Sanne Vedantham, Harish K. Bassa, Cees G. Callingham, Joseph R. Best, William M. J. Liu, Michael C. Magnier, Eugene A. Shimwell, Timothy W. Dupuy, Trent J. |
| author_facet | Bloot, Sanne Vedantham, Harish K. Bassa, Cees G. Callingham, Joseph R. Best, William M. J. Liu, Michael C. Magnier, Eugene A. Shimwell, Timothy W. Dupuy, Trent J. |
| contents | Long-period transients (LPTs) are a new and enigmatic class of objects that produce bright pulsations in the radio, with periods far exceeding those seen in rotationally powered pulsars. The proposed progenitors for LPTs are contested, with white dwarfs or magnetars being likely candidates. Here, we present the discovery of ILT\,J163430+445010, a new LPT detected in a blind search for Stokes\,V transients in the LOFAR Two-Metre Sky Survey. Unusual for LPTs, J1634+44 shows pulses that are 100\% circularly polarised, as well as pulses that are 100\% linearly polarised, with the polarisation state changing from pulse to pulse. We detect 19 pulses in total, each with a total polarisation fraction of $\sim100\%$ and a pulse duration of at most 10\,s. The pulses show a periodicity at $841.24808\pm0.00015$\,s, implying a low duty cycle of $0.012$. J1634+44 has a marginally detected counterpart in the ultraviolet GALEX MIS survey and the ultraviolet/optical UNIONS survey, suggesting that it contains a white dwarf with an effective temperature between 15000\,K and 33000\,K. We do not detect J1634+44 with a deep $J$-band exposure with UKIRT at a $3σ$ AB magnitude limit of 24.7, ruling out a main-sequence star or ultracool dwarf with a spectral type earlier than M7. The pulses from J1634+44 follow a particular pattern, with two pulses being produced every five periods after a waiting time of two or three periods. This pattern could be a result of spin-orbit coupling in a binary system with a 5:2 or 5:3 resonance, where a companion induces beamed radio emission on the white dwarf. The companion is most likely an ultracool dwarf or another white dwarf, making J1634+44 unique among the currently known sample of LPTs. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_05078 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Strongly polarised radio pulses from a new white-dwarf-hosting long-period transient Bloot, Sanne Vedantham, Harish K. Bassa, Cees G. Callingham, Joseph R. Best, William M. J. Liu, Michael C. Magnier, Eugene A. Shimwell, Timothy W. Dupuy, Trent J. High Energy Astrophysical Phenomena Solar and Stellar Astrophysics Long-period transients (LPTs) are a new and enigmatic class of objects that produce bright pulsations in the radio, with periods far exceeding those seen in rotationally powered pulsars. The proposed progenitors for LPTs are contested, with white dwarfs or magnetars being likely candidates. Here, we present the discovery of ILT\,J163430+445010, a new LPT detected in a blind search for Stokes\,V transients in the LOFAR Two-Metre Sky Survey. Unusual for LPTs, J1634+44 shows pulses that are 100\% circularly polarised, as well as pulses that are 100\% linearly polarised, with the polarisation state changing from pulse to pulse. We detect 19 pulses in total, each with a total polarisation fraction of $\sim100\%$ and a pulse duration of at most 10\,s. The pulses show a periodicity at $841.24808\pm0.00015$\,s, implying a low duty cycle of $0.012$. J1634+44 has a marginally detected counterpart in the ultraviolet GALEX MIS survey and the ultraviolet/optical UNIONS survey, suggesting that it contains a white dwarf with an effective temperature between 15000\,K and 33000\,K. We do not detect J1634+44 with a deep $J$-band exposure with UKIRT at a $3σ$ AB magnitude limit of 24.7, ruling out a main-sequence star or ultracool dwarf with a spectral type earlier than M7. The pulses from J1634+44 follow a particular pattern, with two pulses being produced every five periods after a waiting time of two or three periods. This pattern could be a result of spin-orbit coupling in a binary system with a 5:2 or 5:3 resonance, where a companion induces beamed radio emission on the white dwarf. The companion is most likely an ultracool dwarf or another white dwarf, making J1634+44 unique among the currently known sample of LPTs. |
| title | Strongly polarised radio pulses from a new white-dwarf-hosting long-period transient |
| topic | High Energy Astrophysical Phenomena Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2507.05078 |