Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347

B. O'Connor; E. Göǧüş; D. Huppenkothen; C. Kouveliotou; N. Gorgone; L. J. Townsend; A. Calamida; A. Fruchter; D. A.H. Buckley; M. G. Baring; J. A. Kennea; G. Younes; Z. Arzoumanian; E. Bellm; S. B. Cenko; K. Gendreau; J. Granot; C. Hailey; F. Harrison; D. Hartmann; L. Kaper; A. Kutyrev; P. O. Slane; D. Stern; E. Troja; A. J. Van Der Horst; R. A.M.J. Wijers; P. Woudt

doi:10.3847/1538-4357/ac5032

Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347

B. O'Connor
, E. Göǧüş
, D. Huppenkothen
, C. Kouveliotou
, N. Gorgone
, L. J. Townsend
, A. Calamida
, A. Fruchter
, D. A.H. Buckley
, M. G. Baring
, J. A. Kennea
, G. Younes
, Z. Arzoumanian
, E. Bellm
, S. B. Cenko
, K. Gendreau
, J. Granot
, C. Hailey
, F. Harrison
, D. Hartmann

L. Kaper, A. Kutyrev, P. O. Slane, D. Stern, E. Troja, A. J. Van Der Horst, R. A.M.J. Wijers, P. Woudt

פיסיקה

نتاج البحث: نشر في مجلة › مقالة › مراجعة النظراء

ملخص

We report on observations of the candidate Be/X-ray binary (BeXRB) IGR J18219-1347 with the Swift/X-ray Telescope, the Nuclear Spectroscopic Telescope ARray, and the Neutron Star Interior Composition Explorer during Type-I outbursts in 2020 March and June. Our timing analysis revealed the spin period of a neutron star with P spin = 52.46 s. This periodicity, combined with the known orbital period of 72.4 days, indicates that the system is a BeXRB. Furthermore, by comparing the spectral energy distribution of the infrared counterpart to that of known BeXRBs, we confirm this classification and set a distance of approximately 10-15 kpc for the source. The broadband X-ray spectrum (1.5-50 keV) of the source is described by an absorbed power law with a photon index Γ ∼0.5 and a cutoff energy at ∼13 keV.

اللغة الأصلية	الإنجليزيّة
رقم المقال	139
دورية	Astrophysical Journal
مستوى الصوت	927
رقم الإصدار	2
المعرِّفات الرقمية للأشياء	https://doi.org/10.3847/1538-4357/ac5032
حالة النشر	نُشِر - 1 مارس 2022

ملاحظة ببليوغرافية

Publisher Copyright:
© 2022. The Author(s). Published by the American Astronomical Society.

الوصول إلى المستند

10.3847/1538-4357/ac5032

الملفات والروابط الأخرى

Link to publication in Scopus

قم بذكر هذا

O'Connor, B., Göǧüş, E., Huppenkothen, D., Kouveliotou, C., Gorgone, N., Townsend, L. J., Calamida, A., Fruchter, A., Buckley, D. A. H., Baring, M. G., Kennea, J. A., Younes, G., Arzoumanian, Z., Bellm, E., Cenko, S. B., Gendreau, K., Granot, J., Hailey, C., Harrison, F., ... Woudt, P. (2022). Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347. Astrophysical Journal, 927(2), المقال 139. https://doi.org/10.3847/1538-4357/ac5032

@article{f808039941924558b3b8ac3bde7e0bd5,

title = "Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347",

abstract = "We report on observations of the candidate Be/X-ray binary (BeXRB) IGR J18219-1347 with the Swift/X-ray Telescope, the Nuclear Spectroscopic Telescope ARray, and the Neutron Star Interior Composition Explorer during Type-I outbursts in 2020 March and June. Our timing analysis revealed the spin period of a neutron star with P spin = 52.46 s. This periodicity, combined with the known orbital period of 72.4 days, indicates that the system is a BeXRB. Furthermore, by comparing the spectral energy distribution of the infrared counterpart to that of known BeXRBs, we confirm this classification and set a distance of approximately 10-15 kpc for the source. The broadband X-ray spectrum (1.5-50 keV) of the source is described by an absorbed power law with a photon index Γ ∼0.5 and a cutoff energy at ∼13 keV.",

author = "B. O'Connor and E. G{\"o}ǧ{\"u}{\c s} and D. Huppenkothen and C. Kouveliotou and N. Gorgone and Townsend, \{L. J.\} and A. Calamida and A. Fruchter and Buckley, \{D. A.H.\} and Baring, \{M. G.\} and Kennea, \{J. A.\} and G. Younes and Z. Arzoumanian and E. Bellm and Cenko, \{S. B.\} and K. Gendreau and J. Granot and C. Hailey and F. Harrison and D. Hartmann and L. Kaper and A. Kutyrev and Slane, \{P. O.\} and D. Stern and E. Troja and \{Van Der Horst\}, \{A. J.\} and Wijers, \{R. A.M.J.\} and P. Woudt",

note = "Publisher Copyright: {\textcopyright} 2022. The Author(s). Published by the American Astronomical Society.",

year = "2022",

month = mar,

day = "1",

doi = "10.3847/1538-4357/ac5032",

language = "אנגלית",

volume = "927",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

O'Connor, B, Göǧüş, E, Huppenkothen, D, Kouveliotou, C, Gorgone, N, Townsend, LJ, Calamida, A, Fruchter, A, Buckley, DAH, Baring, MG, Kennea, JA, Younes, G, Arzoumanian, Z, Bellm, E, Cenko, SB, Gendreau, K, Granot, J, Hailey, C, Harrison, F, Hartmann, D, Kaper, L, Kutyrev, A, Slane, PO, Stern, D, Troja, E, Van Der Horst, AJ, Wijers, RAMJ & Woudt, P 2022, 'Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347', Astrophysical Journal, المجلد 927, رقم 2, 139. https://doi.org/10.3847/1538-4357/ac5032

TY - JOUR

T1 - Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347

AU - O'Connor, B.

AU - Göǧüş, E.

AU - Huppenkothen, D.

AU - Kouveliotou, C.

AU - Gorgone, N.

AU - Townsend, L. J.

AU - Calamida, A.

AU - Fruchter, A.

AU - Buckley, D. A.H.

AU - Baring, M. G.

AU - Kennea, J. A.

AU - Younes, G.

AU - Arzoumanian, Z.

AU - Bellm, E.

AU - Cenko, S. B.

AU - Gendreau, K.

AU - Granot, J.

AU - Hailey, C.

AU - Harrison, F.

AU - Hartmann, D.

AU - Kaper, L.

AU - Kutyrev, A.

AU - Slane, P. O.

AU - Stern, D.

AU - Troja, E.

AU - Van Der Horst, A. J.

AU - Wijers, R. A.M.J.

AU - Woudt, P.

PY - 2022/3/1

Y1 - 2022/3/1

N2 - We report on observations of the candidate Be/X-ray binary (BeXRB) IGR J18219-1347 with the Swift/X-ray Telescope, the Nuclear Spectroscopic Telescope ARray, and the Neutron Star Interior Composition Explorer during Type-I outbursts in 2020 March and June. Our timing analysis revealed the spin period of a neutron star with P spin = 52.46 s. This periodicity, combined with the known orbital period of 72.4 days, indicates that the system is a BeXRB. Furthermore, by comparing the spectral energy distribution of the infrared counterpart to that of known BeXRBs, we confirm this classification and set a distance of approximately 10-15 kpc for the source. The broadband X-ray spectrum (1.5-50 keV) of the source is described by an absorbed power law with a photon index Γ ∼0.5 and a cutoff energy at ∼13 keV.

AB - We report on observations of the candidate Be/X-ray binary (BeXRB) IGR J18219-1347 with the Swift/X-ray Telescope, the Nuclear Spectroscopic Telescope ARray, and the Neutron Star Interior Composition Explorer during Type-I outbursts in 2020 March and June. Our timing analysis revealed the spin period of a neutron star with P spin = 52.46 s. This periodicity, combined with the known orbital period of 72.4 days, indicates that the system is a BeXRB. Furthermore, by comparing the spectral energy distribution of the infrared counterpart to that of known BeXRBs, we confirm this classification and set a distance of approximately 10-15 kpc for the source. The broadband X-ray spectrum (1.5-50 keV) of the source is described by an absorbed power law with a photon index Γ ∼0.5 and a cutoff energy at ∼13 keV.

UR - https://www.scopus.com/pages/publications/85126595450

U2 - 10.3847/1538-4357/ac5032

DO - 10.3847/1538-4357/ac5032

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:85126595450

SN - 0004-637X

VL - 927

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 139

ER -

Identification of an X-Ray Pulsar in the BeXRB System IGR J18219-1347

ملخص

ملاحظة ببليوغرافية

الوصول إلى المستند

الملفات والروابط الأخرى

بصمة

قم بذكر هذا