PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary

PSR J1953+1844 (i.e., M71E) is a millisecond pulsar in a 53 minute binary orbit discovered by the Five-hundred-meter Aperture Spherical radio Telescope. The mass function from pulsar timing is 2.3 × 10 ^−7 M _⊙ . The possible redback origin of this system has been discussed by Pan et al. We discuss...
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Autor*in:	Z. L. Yang [verfasserIn] J. L. Han [verfasserIn] W. C. Jing [verfasserIn] W. Q. Su [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Binary pulsars X-ray binary stars Low-mass x-ray binary stars Compact binary stars

Übergeordnetes Werk:	In: The Astrophysical Journal Letters - IOP Publishing, 2022, 956(2023), 2, p L39
Übergeordnetes Werk:	volume:956 ; year:2023 ; number:2, p L39

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/2041-8213/acfe6e

Katalog-ID:	DOAJ09268775X

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callnumber-first	Q - Science
author	Z. L. Yang
spellingShingle	Z. L. Yang misc QB460-466 misc Binary pulsars misc X-ray binary stars misc Low-mass x-ray binary stars misc Compact binary stars misc Astrophysics PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary
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topic_title	QB460-466 PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary Binary pulsars X-ray binary stars Low-mass x-ray binary stars Compact binary stars
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title	PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary
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title_sort	psr j1953+1844 probably being the descendant of an ultracompact x-ray binary
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title_auth	PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary
abstract	PSR J1953+1844 (i.e., M71E) is a millisecond pulsar in a 53 minute binary orbit discovered by the Five-hundred-meter Aperture Spherical radio Telescope. The mass function from pulsar timing is 2.3 × 10 ^−7 M _⊙ . The possible redback origin of this system has been discussed by Pan et al. We discuss here an alternative evolution track for this binary system, namely that PSR J1953+1844 is a descendant of an ultracompact X-ray binary (UCXB), which has a hydrogen-poor donor accreting onto a neutron star (NS) with an orbital period of ≤1 hr. We noticed that some UCXB systems hold an accreting millisecond X-ray pulsar (AMXP) and a donor with a mass of about 0.01 M _⊙ . M71E has a very similar orbit to those of AMXPs, indicating that it might be evolved from a UCXB similar to PSR J1653–0158. The companion star of M71E should be significantly bloated and it most probably has a carbon and oxygen composition, otherwise a low inclination angle of the orbit is required for a helium companion. The discovery of this M71E binary system may shed light on when and how an NS in a UCXB turns into a radio pulsar.
abstractGer	PSR J1953+1844 (i.e., M71E) is a millisecond pulsar in a 53 minute binary orbit discovered by the Five-hundred-meter Aperture Spherical radio Telescope. The mass function from pulsar timing is 2.3 × 10 ^−7 M _⊙ . The possible redback origin of this system has been discussed by Pan et al. We discuss here an alternative evolution track for this binary system, namely that PSR J1953+1844 is a descendant of an ultracompact X-ray binary (UCXB), which has a hydrogen-poor donor accreting onto a neutron star (NS) with an orbital period of ≤1 hr. We noticed that some UCXB systems hold an accreting millisecond X-ray pulsar (AMXP) and a donor with a mass of about 0.01 M _⊙ . M71E has a very similar orbit to those of AMXPs, indicating that it might be evolved from a UCXB similar to PSR J1653–0158. The companion star of M71E should be significantly bloated and it most probably has a carbon and oxygen composition, otherwise a low inclination angle of the orbit is required for a helium companion. The discovery of this M71E binary system may shed light on when and how an NS in a UCXB turns into a radio pulsar.
abstract_unstemmed	PSR J1953+1844 (i.e., M71E) is a millisecond pulsar in a 53 minute binary orbit discovered by the Five-hundred-meter Aperture Spherical radio Telescope. The mass function from pulsar timing is 2.3 × 10 ^−7 M _⊙ . The possible redback origin of this system has been discussed by Pan et al. We discuss here an alternative evolution track for this binary system, namely that PSR J1953+1844 is a descendant of an ultracompact X-ray binary (UCXB), which has a hydrogen-poor donor accreting onto a neutron star (NS) with an orbital period of ≤1 hr. We noticed that some UCXB systems hold an accreting millisecond X-ray pulsar (AMXP) and a donor with a mass of about 0.01 M _⊙ . M71E has a very similar orbit to those of AMXPs, indicating that it might be evolved from a UCXB similar to PSR J1653–0158. The companion star of M71E should be significantly bloated and it most probably has a carbon and oxygen composition, otherwise a low inclination angle of the orbit is required for a helium companion. The discovery of this M71E binary system may shed light on when and how an NS in a UCXB turns into a radio pulsar.
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PSR J1953+1844 Probably Being the Descendant of an Ultracompact X-Ray Binary

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