Absorption features in spectra of magnetized neutron stars

V. Suleimanov, V. Hambaryan, A. Y. Potekhin, G. G. Pavlov, M. Van Adelsberg, R. Neuhäuser, K. Werner

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The X-ray spectra of some magnetized isolated neutron stars (NSs) show absorption features with equivalent widths (EWs) of 50-200 eV, whose nature is not yet well known. To explain the prominent absorption features in the soft X-ray spectra of the highly magnetized (B∼1014G) X-ray dim isolated NSs (XDINSs), we theoretically investigate different NS local surface models, including naked condensed iron surfaces and partially ionized hydrogen model atmospheres, with semi-infinite and thin atmospheres above the condensed surface. We also developed a code for computing light curves and integral emergent spectra of magnetized neutron stars with various temperature and magnetic field distributions over the NS surface. We compare the general properties of the computed and observed light curves and integral spectra for XDINS RBS 1223 and conclude that the observations can be explained by a thin hydrogen atmosphere above the condensed iron surface, while the presence of a strong toroidal magnetic field component on the XDINS surface is unlikely. We suggest that the harmonically spaced absorption features in the soft X-ray spectrum of the central compact object (CCO) 1E 1207.4-5209 (hereafter 1E 1207) correspond to peaks in the energy dependence of the free-free opacity in a quantizing magnetic field, known as quantum oscillations. To explore observable properties of these quantum oscillations, we calculate models of hydrogen NS atmospheres with B∼1010-1011G (i.e., electron cyclotron energy Ec,e∼0.1-1keV) and Teff=1-3MK. Such conditions are thought to be typical for 1E 1207. We show that observable features at the electron cyclotron harmonics with EWs ≈100-200eV can arise due to these quantum oscillations.

Original languageEnglish (US)
Title of host publicationAstrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar
Pages119-122
Number of pages4
DOIs
StatePublished - Oct 5 2011
EventAstrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar - Cesme, Izmir, Turkey
Duration: Aug 2 2010Aug 6 2010

Publication series

NameAIP Conference Proceedings
Volume1379
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherAstrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar
CountryTurkey
CityCesme, Izmir
Period8/2/108/6/10

Fingerprint

neutron stars
atmospheres
x rays
oscillations
light curve
cyclotrons
hydrogen
magnetic fields
iron
opacity
temperature distribution
electrons
harmonics
energy

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Suleimanov, V., Hambaryan, V., Potekhin, A. Y., Pavlov, G. G., Van Adelsberg, M., Neuhäuser, R., & Werner, K. (2011). Absorption features in spectra of magnetized neutron stars. In Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar (pp. 119-122). (AIP Conference Proceedings; Vol. 1379). https://doi.org/10.1063/1.3629497
Suleimanov, V. ; Hambaryan, V. ; Potekhin, A. Y. ; Pavlov, G. G. ; Van Adelsberg, M. ; Neuhäuser, R. ; Werner, K. / Absorption features in spectra of magnetized neutron stars. Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar. 2011. pp. 119-122 (AIP Conference Proceedings).
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Suleimanov, V, Hambaryan, V, Potekhin, AY, Pavlov, GG, Van Adelsberg, M, Neuhäuser, R & Werner, K 2011, Absorption features in spectra of magnetized neutron stars. in Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar. AIP Conference Proceedings, vol. 1379, pp. 119-122, Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar, Cesme, Izmir, Turkey, 8/2/10. https://doi.org/10.1063/1.3629497

Absorption features in spectra of magnetized neutron stars. / Suleimanov, V.; Hambaryan, V.; Potekhin, A. Y.; Pavlov, G. G.; Van Adelsberg, M.; Neuhäuser, R.; Werner, K.

Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar. 2011. p. 119-122 (AIP Conference Proceedings; Vol. 1379).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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N2 - The X-ray spectra of some magnetized isolated neutron stars (NSs) show absorption features with equivalent widths (EWs) of 50-200 eV, whose nature is not yet well known. To explain the prominent absorption features in the soft X-ray spectra of the highly magnetized (B∼1014G) X-ray dim isolated NSs (XDINSs), we theoretically investigate different NS local surface models, including naked condensed iron surfaces and partially ionized hydrogen model atmospheres, with semi-infinite and thin atmospheres above the condensed surface. We also developed a code for computing light curves and integral emergent spectra of magnetized neutron stars with various temperature and magnetic field distributions over the NS surface. We compare the general properties of the computed and observed light curves and integral spectra for XDINS RBS 1223 and conclude that the observations can be explained by a thin hydrogen atmosphere above the condensed iron surface, while the presence of a strong toroidal magnetic field component on the XDINS surface is unlikely. We suggest that the harmonically spaced absorption features in the soft X-ray spectrum of the central compact object (CCO) 1E 1207.4-5209 (hereafter 1E 1207) correspond to peaks in the energy dependence of the free-free opacity in a quantizing magnetic field, known as quantum oscillations. To explore observable properties of these quantum oscillations, we calculate models of hydrogen NS atmospheres with B∼1010-1011G (i.e., electron cyclotron energy Ec,e∼0.1-1keV) and Teff=1-3MK. Such conditions are thought to be typical for 1E 1207. We show that observable features at the electron cyclotron harmonics with EWs ≈100-200eV can arise due to these quantum oscillations.

AB - The X-ray spectra of some magnetized isolated neutron stars (NSs) show absorption features with equivalent widths (EWs) of 50-200 eV, whose nature is not yet well known. To explain the prominent absorption features in the soft X-ray spectra of the highly magnetized (B∼1014G) X-ray dim isolated NSs (XDINSs), we theoretically investigate different NS local surface models, including naked condensed iron surfaces and partially ionized hydrogen model atmospheres, with semi-infinite and thin atmospheres above the condensed surface. We also developed a code for computing light curves and integral emergent spectra of magnetized neutron stars with various temperature and magnetic field distributions over the NS surface. We compare the general properties of the computed and observed light curves and integral spectra for XDINS RBS 1223 and conclude that the observations can be explained by a thin hydrogen atmosphere above the condensed iron surface, while the presence of a strong toroidal magnetic field component on the XDINS surface is unlikely. We suggest that the harmonically spaced absorption features in the soft X-ray spectrum of the central compact object (CCO) 1E 1207.4-5209 (hereafter 1E 1207) correspond to peaks in the energy dependence of the free-free opacity in a quantizing magnetic field, known as quantum oscillations. To explore observable properties of these quantum oscillations, we calculate models of hydrogen NS atmospheres with B∼1010-1011G (i.e., electron cyclotron energy Ec,e∼0.1-1keV) and Teff=1-3MK. Such conditions are thought to be typical for 1E 1207. We show that observable features at the electron cyclotron harmonics with EWs ≈100-200eV can arise due to these quantum oscillations.

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Suleimanov V, Hambaryan V, Potekhin AY, Pavlov GG, Van Adelsberg M, Neuhäuser R et al. Absorption features in spectra of magnetized neutron stars. In Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar. 2011. p. 119-122. (AIP Conference Proceedings). https://doi.org/10.1063/1.3629497