Search for a Radio Pulsar in the Remnant of Supernova 1987A

Abstract

We have observed the remnant of supernova SN~1987A (SNR~1987A), located in the Large Magellanic Cloud (LMC), to search for periodic and/or transient radio emission with the Parkes 64\,m-diameter radio telescope. We found no evidence of a radio pulsar in our periodicity search and derived 8$\sigma$ upper bounds on the flux density of any such source of $31\mu$Jy at 1.4~GHz and $21\mu$Jy at 3~GHz. Four candidate transient events were detected with greater than $7\sigma$ significance, with dispersion measures (DMs) in the range 150 to 840\,cm${}^{-3}$pc. For two of them, we found a second pulse at slightly lower significance. However, we cannot at present conclude that any of these are associated with a pulsar in SNR~1987A. As a check on the system, we also observed PSR~B0540$-$69, a young pulsar which also lies in the LMC. We found eight giant pulses at the DM of this pulsar. We discuss the implications of these results for models of the supernova remnant, neutron star formation and pulsar evolution.

arXiv comment7 pages, 3 figures, 2 tables. Accepted for publication in MNRAS

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• High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta
• Parameter estimation with gravitational waves
• Exciting Prospects for Detecting Late-Time Neutrinos from Core-Collapse Supernovae
• The 30-Year Search for the Compact Object in SN 1987A
• A new fast radio burst in the datasets containing the Lorimer burst
• Parkes transient events: I. Database of single pulses, initial results and missing FRBs
• Applying saliency-map analysis in searches for pulsars and fast radio bursts
• Consequences of Fine-Tuning for Fifth Force Searches
• A search for radio pulsars in five nearby supernova remnants
• The TRAPUM Large Magellanic Cloud pulsar survey with MeerKAT I: Survey setup and first seven pulsar discoveries
• No Pulsar Detected in Reprocessed Archival Parkes Observations of SNR 1987A