Searching for supergiant fast X-ray transients with Swift

P. Romano, E. Bozzo, P. Esposito, B. Sbarufatti, F. Haberl, G. Ponti, P. D'Avanzo, L. Ducci, A. Segreto, C. Jin, N. Masetti, M. Del Santo, S. Campana, V. Mangano

Resultado de la investigación: Article

Resumen

Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources: IGR J17407-2808, 2XMM J185114.3-000004, and IGR J18175-2419, whose X-ray characteristics qualify them as candidate SFXT, to explore their properties and test whether they are consistent with an SFXT nature. Since IGR J17407-2808 and 2XMM J185114.3-000004 triggered the Burst Alert Telescope on board Swift, the Swift data enable us to provide their first arcsecond localisations, leading to an unequivocal identification of the source CXOU J174042.0-280724 as the soft X-ray counterpart of IGR J17407-2808, as well as their first broadband spectra, which can be fit with models generally describing accreting neutron stars in HMXBs. While still lacking optical spectroscopy to assess the spectral type of the companion, we propose 2XMM J185114.3-000004 as a very strong SFXT candidate. The nature of IGR J17407-2808 remains, instead, more uncertain. Its broadband properties cannot exclude the fact that the emission originates from either an HMXB (and in that case, an SFXT) or, more likely, a low-mass X-ray binary. Finally, based on the deep non-detection in our XRT monitoring campaign and a careful reanalysis of the original INTEGRAL data in which the discovery of the source was first reported, we show that IGR J18175-2419 is likely a spurious detection.

Idioma originalEnglish
Número de artículoA96
PublicaciónAstronomy and Astrophysics
Volumen593
DOI
EstadoPublished - 1 sep 2016

Huella dactilar

x rays
neutron stars
broadband
bursts
spectroscopy
telescopes
monitoring

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Citar esto

Romano, P., Bozzo, E., Esposito, P., Sbarufatti, B., Haberl, F., Ponti, G., ... Mangano, V. (2016). Searching for supergiant fast X-ray transients with Swift. Astronomy and Astrophysics, 593, [A96]. https://doi.org/10.1051/0004-6361/201628808
Romano, P. ; Bozzo, E. ; Esposito, P. ; Sbarufatti, B. ; Haberl, F. ; Ponti, G. ; D'Avanzo, P. ; Ducci, L. ; Segreto, A. ; Jin, C. ; Masetti, N. ; Del Santo, M. ; Campana, S. ; Mangano, V. / Searching for supergiant fast X-ray transients with Swift. En: Astronomy and Astrophysics. 2016 ; Vol. 593.
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abstract = "Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources: IGR J17407-2808, 2XMM J185114.3-000004, and IGR J18175-2419, whose X-ray characteristics qualify them as candidate SFXT, to explore their properties and test whether they are consistent with an SFXT nature. Since IGR J17407-2808 and 2XMM J185114.3-000004 triggered the Burst Alert Telescope on board Swift, the Swift data enable us to provide their first arcsecond localisations, leading to an unequivocal identification of the source CXOU J174042.0-280724 as the soft X-ray counterpart of IGR J17407-2808, as well as their first broadband spectra, which can be fit with models generally describing accreting neutron stars in HMXBs. While still lacking optical spectroscopy to assess the spectral type of the companion, we propose 2XMM J185114.3-000004 as a very strong SFXT candidate. The nature of IGR J17407-2808 remains, instead, more uncertain. Its broadband properties cannot exclude the fact that the emission originates from either an HMXB (and in that case, an SFXT) or, more likely, a low-mass X-ray binary. Finally, based on the deep non-detection in our XRT monitoring campaign and a careful reanalysis of the original INTEGRAL data in which the discovery of the source was first reported, we show that IGR J18175-2419 is likely a spurious detection.",
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Romano, P, Bozzo, E, Esposito, P, Sbarufatti, B, Haberl, F, Ponti, G, D'Avanzo, P, Ducci, L, Segreto, A, Jin, C, Masetti, N, Del Santo, M, Campana, S & Mangano, V 2016, 'Searching for supergiant fast X-ray transients with Swift', Astronomy and Astrophysics, vol. 593, A96. https://doi.org/10.1051/0004-6361/201628808

Searching for supergiant fast X-ray transients with Swift. / Romano, P.; Bozzo, E.; Esposito, P.; Sbarufatti, B.; Haberl, F.; Ponti, G.; D'Avanzo, P.; Ducci, L.; Segreto, A.; Jin, C.; Masetti, N.; Del Santo, M.; Campana, S.; Mangano, V.

En: Astronomy and Astrophysics, Vol. 593, A96, 01.09.2016.

Resultado de la investigación: Article

TY - JOUR

T1 - Searching for supergiant fast X-ray transients with Swift

AU - Romano, P.

AU - Bozzo, E.

AU - Esposito, P.

AU - Sbarufatti, B.

AU - Haberl, F.

AU - Ponti, G.

AU - D'Avanzo, P.

AU - Ducci, L.

AU - Segreto, A.

AU - Jin, C.

AU - Masetti, N.

AU - Del Santo, M.

AU - Campana, S.

AU - Mangano, V.

PY - 2016/9/1

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N2 - Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources: IGR J17407-2808, 2XMM J185114.3-000004, and IGR J18175-2419, whose X-ray characteristics qualify them as candidate SFXT, to explore their properties and test whether they are consistent with an SFXT nature. Since IGR J17407-2808 and 2XMM J185114.3-000004 triggered the Burst Alert Telescope on board Swift, the Swift data enable us to provide their first arcsecond localisations, leading to an unequivocal identification of the source CXOU J174042.0-280724 as the soft X-ray counterpart of IGR J17407-2808, as well as their first broadband spectra, which can be fit with models generally describing accreting neutron stars in HMXBs. While still lacking optical spectroscopy to assess the spectral type of the companion, we propose 2XMM J185114.3-000004 as a very strong SFXT candidate. The nature of IGR J17407-2808 remains, instead, more uncertain. Its broadband properties cannot exclude the fact that the emission originates from either an HMXB (and in that case, an SFXT) or, more likely, a low-mass X-ray binary. Finally, based on the deep non-detection in our XRT monitoring campaign and a careful reanalysis of the original INTEGRAL data in which the discovery of the source was first reported, we show that IGR J18175-2419 is likely a spurious detection.

AB - Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources: IGR J17407-2808, 2XMM J185114.3-000004, and IGR J18175-2419, whose X-ray characteristics qualify them as candidate SFXT, to explore their properties and test whether they are consistent with an SFXT nature. Since IGR J17407-2808 and 2XMM J185114.3-000004 triggered the Burst Alert Telescope on board Swift, the Swift data enable us to provide their first arcsecond localisations, leading to an unequivocal identification of the source CXOU J174042.0-280724 as the soft X-ray counterpart of IGR J17407-2808, as well as their first broadband spectra, which can be fit with models generally describing accreting neutron stars in HMXBs. While still lacking optical spectroscopy to assess the spectral type of the companion, we propose 2XMM J185114.3-000004 as a very strong SFXT candidate. The nature of IGR J17407-2808 remains, instead, more uncertain. Its broadband properties cannot exclude the fact that the emission originates from either an HMXB (and in that case, an SFXT) or, more likely, a low-mass X-ray binary. Finally, based on the deep non-detection in our XRT monitoring campaign and a careful reanalysis of the original INTEGRAL data in which the discovery of the source was first reported, we show that IGR J18175-2419 is likely a spurious detection.

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KW - X-rays: individuals: 2XMM J185114.3-000004

KW - X-rays: individuals: IGR J17407-2808

KW - X-rays: individuals: IGR J18175-2419

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Romano P, Bozzo E, Esposito P, Sbarufatti B, Haberl F, Ponti G y otros. Searching for supergiant fast X-ray transients with Swift. Astronomy and Astrophysics. 2016 sep 1;593. A96. https://doi.org/10.1051/0004-6361/201628808