Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321
We report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the γ -ray source 3FGL J0212.5+5320 using the Robert C. Byrd Green Bank Telescope (GBT) with the Breakthrough Listen backend at L band. Over a seven month period,...
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IOP Publishing
2023-01-01
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Online Access: | https://doi.org/10.3847/1538-4357/acdc23 |
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author | Karen I. Perez Slavko Bogdanov Jules P. Halpern Vishal Gajjar |
author_facet | Karen I. Perez Slavko Bogdanov Jules P. Halpern Vishal Gajjar |
author_sort | Karen I. Perez |
collection | DOAJ |
description | We report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the γ -ray source 3FGL J0212.5+5320 using the Robert C. Byrd Green Bank Telescope (GBT) with the Breakthrough Listen backend at L band. Over a seven month period, five pointings were made near inferior conjunction of the pulsar in its 20.9 hr orbit, resulting in two detections, lasting 12 and 42 minutes. The pulsar dispersion measure (DM) of 25.7 pc cm ^−3 corresponds to a distance of 1.15 kpc in the NE2001 Galactic electron density model, consistent with the Gaia parallax distance of 1.16 ± 0.03 kpc for the companion star. We suspect the pulsar experiences wide orbital eclipses, similar to other redbacks, as well as scintillation and DM delays caused by its interaction with its companion and surroundings. Although the pulsar was only detected over ≈3.7% of the orbit, its measured acceleration is consistent with published binary parameters from optical radial velocity spectroscopy and light-curve modeling of the companion star, and it provides a more precise mass ratio and a projected semimajor axis for the pulsar orbit. We also obtained a refined optical photometric orbit ephemeris, and observed variability of the tidally distorted companion over 7 yr. A hard X-ray light curve from NuSTAR shows expected orbit-modulated emission from the intrabinary shock. The pulsar parameters and photometric ephemeris greatly restrict the parameter space required to search for a coherent timing solution including pulsar spin-down rate, either using Fermi γ -rays or further radio pulse detections. |
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issn | 1538-4357 |
language | English |
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series | The Astrophysical Journal |
spelling | doaj.art-a4a133932bdf46749a9b8a0191ac9fa72023-09-03T12:34:26ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01952215010.3847/1538-4357/acdc23Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321Karen I. Perez0https://orcid.org/0000-0002-6341-4548Slavko Bogdanov1https://orcid.org/0000-0002-9870-2742Jules P. Halpern2https://orcid.org/0000-0003-4814-2377Vishal Gajjar3https://orcid.org/0000-0002-8604-106XDepartment of Astronomy, Columbia University , 550 West 120th Street, New York, NY 10027, USAColumbia Astrophysics Laboratory, Columbia University , 550 West 120th Street, New York, NY 10027, USADepartment of Astronomy, Columbia University , 550 West 120th Street, New York, NY 10027, USA; Columbia Astrophysics Laboratory, Columbia University , 550 West 120th Street, New York, NY 10027, USADepartment of Astronomy, University of California Berkeley , Berkeley CA 94720, USAWe report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the γ -ray source 3FGL J0212.5+5320 using the Robert C. Byrd Green Bank Telescope (GBT) with the Breakthrough Listen backend at L band. Over a seven month period, five pointings were made near inferior conjunction of the pulsar in its 20.9 hr orbit, resulting in two detections, lasting 12 and 42 minutes. The pulsar dispersion measure (DM) of 25.7 pc cm ^−3 corresponds to a distance of 1.15 kpc in the NE2001 Galactic electron density model, consistent with the Gaia parallax distance of 1.16 ± 0.03 kpc for the companion star. We suspect the pulsar experiences wide orbital eclipses, similar to other redbacks, as well as scintillation and DM delays caused by its interaction with its companion and surroundings. Although the pulsar was only detected over ≈3.7% of the orbit, its measured acceleration is consistent with published binary parameters from optical radial velocity spectroscopy and light-curve modeling of the companion star, and it provides a more precise mass ratio and a projected semimajor axis for the pulsar orbit. We also obtained a refined optical photometric orbit ephemeris, and observed variability of the tidally distorted companion over 7 yr. A hard X-ray light curve from NuSTAR shows expected orbit-modulated emission from the intrabinary shock. The pulsar parameters and photometric ephemeris greatly restrict the parameter space required to search for a coherent timing solution including pulsar spin-down rate, either using Fermi γ -rays or further radio pulse detections.https://doi.org/10.3847/1538-4357/acdc23Millisecond pulsarsBinary pulsarsRadio pulsarsRotation-powered pulsarsPulsarsNeutron stars |
spellingShingle | Karen I. Perez Slavko Bogdanov Jules P. Halpern Vishal Gajjar Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 The Astrophysical Journal Millisecond pulsars Binary pulsars Radio pulsars Rotation-powered pulsars Pulsars Neutron stars |
title | Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 |
title_full | Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 |
title_fullStr | Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 |
title_full_unstemmed | Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 |
title_short | Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321 |
title_sort | green bank telescope discovery of the redback binary millisecond pulsar psr j0212 5321 |
topic | Millisecond pulsars Binary pulsars Radio pulsars Rotation-powered pulsars Pulsars Neutron stars |
url | https://doi.org/10.3847/1538-4357/acdc23 |
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