PSR J1947−1120: A New Huntsman Millisecond Pulsar Binary

Abstract We present the discovery of PSR J1947–1120, a new huntsman millisecond pulsar with a red giant companion star in a 10.3 day orbit. This pulsar was found via optical, X-ray, and radio follow-up of the previously unassociated γ -ray source 4FGL J1947.6–1121. PSR J1947–1120 is the second confirmed pulsar in the huntsman class and establishes this as a bona fide subclass of millisecond pulsars. We use MESA models to show that huntsman pulsars can be naturally explained as neutron star binaries whose secondaries are currently in the “red bump” region of the red giant branch, temporarily underfilling their Roche lobes and hence halting mass transfer. Huntsman pulsars offer a new view of the formation of typical millisecond pulsars, allowing novel constraints on the efficiency of mass transfer and recycling at an intermediate stage in the process.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2025-02-07
DOI
https://doi.org/10.3847/1538-4357/ada897
Citations
5
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
5.77

Funders

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article

PSR J1947−1120: A New Huntsman Millisecond Pulsar Binary

I. Molina, Jay Strader, M. A. McLaughlin, Ryan T Urquhart et al.
5 citations
The Astrophysical Journal
Pulsars and Gravitational Waves Research
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article

PSR J1947−1120: A New Huntsman Millisecond Pulsar Binary

I. Molina, Jay Strader, M. A. McLaughlin, Ryan T Urquhart, E. Aydi, Teresa Panurach, Paul S. Ray, Laura B. Chomiuk, Samuel J. Swihart, J. S. Deneva, Eric C. Bellm, Kristen C. Dage, K. V. Sokolovsky, Megan E. DeCesar
article en
5 citations

Abstract

Abstract We present the discovery of PSR J1947–1120, a new huntsman millisecond pulsar with a red giant companion star in a 10.3 day orbit. This pulsar was found via optical, X-ray, and radio follow-up of the previously unassociated γ -ray source 4FGL J1947.6–1121. PSR J1947–1120 is the second confirmed pulsar in the huntsman class and establishes this as a bona fide subclass of millisecond pulsars. We use MESA models to show that huntsman pulsars can be naturally explained as neutron star binaries whose secondaries are currently in the “red bump” region of the red giant branch, temporarily underfilling their Roche lobes and hence halting mass transfer. Huntsman pulsars offer a new view of the formation of typical millisecond pulsars, allowing novel constraints on the efficiency of mass transfer and recycling at an intermediate stage in the process.

The Astrophysical JournalVol. 980(1)
David and Lucile Packard Foundation, National Aeronautics and Space Administration
Openalex Percentile: Top 5%
Pulsars and Gravitational Waves Research
5.77
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