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NICER discovery that SRGA J144459.2-604207 is an accreting millisecond X-ray pulsar

NICER discovery that SRGA J144459.2-604207 is an accreting millisecond X-ray pulsar
NICER discovery that SRGA J144459.2-604207 is an accreting millisecond X-ray pulsar
We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2−604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a 4 week long outburst starting on 2024 February 15. The AMXP resides in a 5.22 hr binary, orbiting a low-mass companion donor with Md > 0.1 M⊙. We report on the temporal and spectral properties from NICER observations during the early days of the outburst, from 2024 February 21 through 2024 February 23, during which NICER also detected a type I X-ray burst that exhibited a plateau lasting ∼6 s. The spectra of the persistent emission were well described by an absorbed thermal blackbody and power-law model, with blackbody temperature kT ≈ 0.9 keV and power-law photon index Γ ≈ 1.9. Time-resolved burst spectroscopy confirmed the thermonuclear nature of the burst, where an additional blackbody component reached a maximum temperature of nearly kT ≈ 3 keV at the peak of the burst. We discuss the nature of the companion as well as the type I X-ray burst.
astro-ph.HE
2041-8213
Ng, Mason
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Ray, Paul S.
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Sanna, Andrea
f132c9e7-4e3e-4d3a-84a3-85f5724b5f4d
Strohmayer, Tod E.
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Papitto, Alessandro
ce86b717-5c62-42a1-8b22-5ff0aa4f28b6
Illiano, Giulia
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Albayati, Arianna C.
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Altamirano, Diego
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Boztepe, Tuğba
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Güver, Tolga
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Chakrabarty, Deepto
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Arzoumanian, Zaven
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Buisson, D. J. K.
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Ferrara, Elizabeth C.
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Gendreau, Keith C.
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Guillot, Sebastien
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Hare, Jeremy
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Jaisawal, Gaurava K.
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Malacaria, Christian
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Wolff, Michael T.
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Ng, Mason
1ea126a4-d65f-4ea4-a97b-dd8620d745e4
Ray, Paul S.
1af653fd-166e-4aae-b7cd-7068f0c4bbcf
Sanna, Andrea
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Strohmayer, Tod E.
e1a6de84-d23d-43de-b33e-2d49c4a5daa7
Papitto, Alessandro
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Illiano, Giulia
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Albayati, Arianna C.
a37b49d4-f72d-407f-b7dc-ee3ce0dccbd2
Altamirano, Diego
d5ccdb09-0b71-4303-9538-05b467be075b
Boztepe, Tuğba
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Güver, Tolga
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Chakrabarty, Deepto
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Arzoumanian, Zaven
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Buisson, D. J. K.
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Ferrara, Elizabeth C.
65915a6a-f7d3-45a9-8271-7efe0109841c
Gendreau, Keith C.
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Guillot, Sebastien
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Hare, Jeremy
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Jaisawal, Gaurava K.
ee3d96c5-843a-4802-8ae4-c1cfd211ec6f
Malacaria, Christian
0fda98ec-bedd-44ed-bb32-923754440d89
Wolff, Michael T.
bf1dbc0e-28c1-4b44-aa86-71111986c73b

Ng, Mason, Ray, Paul S., Sanna, Andrea, Strohmayer, Tod E., Papitto, Alessandro, Illiano, Giulia, Albayati, Arianna C., Altamirano, Diego, Boztepe, Tuğba, Güver, Tolga, Chakrabarty, Deepto, Arzoumanian, Zaven, Buisson, D. J. K., Ferrara, Elizabeth C., Gendreau, Keith C., Guillot, Sebastien, Hare, Jeremy, Jaisawal, Gaurava K., Malacaria, Christian and Wolff, Michael T. (2024) NICER discovery that SRGA J144459.2-604207 is an accreting millisecond X-ray pulsar. The Astrophysical Journal Letters, 968 (1), [L7]. (doi:10.3847/2041-8213/ad4edb).

Record type: Article

Abstract

We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2−604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a 4 week long outburst starting on 2024 February 15. The AMXP resides in a 5.22 hr binary, orbiting a low-mass companion donor with Md > 0.1 M⊙. We report on the temporal and spectral properties from NICER observations during the early days of the outburst, from 2024 February 21 through 2024 February 23, during which NICER also detected a type I X-ray burst that exhibited a plateau lasting ∼6 s. The spectra of the persistent emission were well described by an absorbed thermal blackbody and power-law model, with blackbody temperature kT ≈ 0.9 keV and power-law photon index Γ ≈ 1.9. Time-resolved burst spectroscopy confirmed the thermonuclear nature of the burst, where an additional blackbody component reached a maximum temperature of nearly kT ≈ 3 keV at the peak of the burst. We discuss the nature of the companion as well as the type I X-ray burst.

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Accepted/In Press date: 14 May 2024
e-pub ahead of print date: 6 June 2024
Keywords: astro-ph.HE

Identifiers

Local EPrints ID: 496296
URI: http://eprints.soton.ac.uk/id/eprint/496296
ISSN: 2041-8213
PURE UUID: 57007af7-cf9a-47a6-b8bd-73f4c50dc401
ORCID for Diego Altamirano: ORCID iD orcid.org/0000-0002-3422-0074

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Date deposited: 11 Dec 2024 17:34
Last modified: 12 Dec 2024 02:46

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Contributors

Author: Mason Ng
Author: Paul S. Ray
Author: Andrea Sanna
Author: Tod E. Strohmayer
Author: Alessandro Papitto
Author: Giulia Illiano
Author: Tuğba Boztepe
Author: Tolga Güver
Author: Deepto Chakrabarty
Author: Zaven Arzoumanian
Author: D. J. K. Buisson
Author: Elizabeth C. Ferrara
Author: Keith C. Gendreau
Author: Sebastien Guillot
Author: Jeremy Hare
Author: Gaurava K. Jaisawal
Author: Christian Malacaria
Author: Michael T. Wolff

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