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A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RXJ0822–4300

De Luca, A; Salvetti, D; Sartori, A; Esposito, P; Tiengo, A; Zane, S; Turolla, R; ... Bignami, GF; + view all (2012) A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RXJ0822–4300. Monthly Notices of the Royal Astronomical Society: Letters , 421 (1) L72-L76. 10.1111/j.1745-3933.2011.01209.x. Green open access

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Abstract

RX J0822−4300 is the central compact object associated with the Puppis A supernova remnant. Previous X-ray observations suggested RX J0822−4300 to be a young neutron star with a weak dipole field and a peculiar surface temperature distribution dominated by two antipodal spots with different temperatures and sizes. An emission line at 0.8 keV was also detected. We performed a very deep (130-ks) observation with XMM–Newton, which allowed us to study in detail the phase-resolved properties of RX J0822−4300. Our new data confirm the existence of a narrow spectral feature, best modelled as an emission line, only seen in the ‘soft’-phase interval – when the cooler region is best aligned to the line of sight. Surprisingly, comparison of our recent observations to the older ones yields evidence for a variation in the emission-line component, which can be modelled as a decrease in the central energy from ∼0.80 keV in 2001 to ∼0.73 keV in 2009–10. The line could be generated via cyclotron scattering of thermal photons in an optically-thin layer of gas, or, alternatively, it could originate in low-rate accretion by a debris disc. In any case, a variation in energy, pointing to a variation of the magnetic field in the line-emitting region, cannot be easily accounted for.

Type: Article
Title: A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RXJ0822–4300
Open access status: An open access version is available from UCL Discovery
DOI: 10.1111/j.1745-3933.2011.01209.x
Publisher version: https://doi.org/10.1111/j.1745-3933.2011.01209.x
Language: English
Additional information: This is the published version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: stars: neutron; pulsars: general; X-rays: individual: RX J0822−4300
UCL classification: UCL
UCL > Provost and Vice Provost Offices
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1333411
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