Time-resolved spectroscopy of the M15 X-ray binary AC211/X2127+119
dc.contributor.author | Torres, Manuel Angel Perez | |
dc.contributor.author | Callanan, Paul J. | |
dc.contributor.author | Garcia, M. R. | |
dc.date.accessioned | 2017-11-07T09:38:59Z | |
dc.date.available | 2017-11-07T09:38:59Z | |
dc.date.issued | 2003 | |
dc.description.abstract | We present time-resolved spectroscopy acquired during two epochs (spaced apart by similar to15 d) of the eclipsing low-mass X-ray binary AC211/X2127+119 in the globular cluster M15. The spectra show variations in the He iilambda4686 emission line not only modulated on the orbital period, but also on time-scales of a few days. During the first epoch of observation, the emission line shows a strong S -wave superimposed on the average double-peaked profile. The line exhibits no evidence of rotational disturbance at the orbital phases when the eclipse is observed in the optical continuum. During the second epoch, no double-peak or S -wave component is present. The He i absorption lines detected by other authors are not present in our spectra. A Doppler image of He iilambda4686 for the first epoch supports the presence of the accretion disc. No hotspot is detected, although enhanced emission at V-X = 30 km s(-1) , V-Y = 160 km s(-1) is observed. We discuss the implications of this emission in the context of an X-ray heated donor star, in which case a high mass ratio and neutron star primary are implied. Finally, we speculate on the possibility of a misaligned secondary star in AC211. | en |
dc.description.status | Peer reviewed | en |
dc.description.version | Published Version | en |
dc.format.mimetype | application/pdf | en |
dc.identifier.citation | Torres, M. A. P., Callanan, P. J. and Garcia, M. R. (2003) 'Time-resolved spectroscopy of the M15 X-ray binary AC211/X2127+119', Monthly Notices of the Royal Astronomical Society, 341(4), pp. 1231-1238. doi:10.1046/j.1365-8711.2003.06486.x | en |
dc.identifier.doi | 10.1046/j.1365-8711.2003.06486.x | |
dc.identifier.endpage | 1238 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issued | 4 | |
dc.identifier.journaltitle | Monthly Notices of the Royal Astronomical Society | en |
dc.identifier.startpage | 1231 | |
dc.identifier.uri | https://hdl.handle.net/10468/4988 | |
dc.identifier.volume | 341 | |
dc.language.iso | en | en |
dc.publisher | Oxford University Press | en |
dc.relation.uri | https://academic.oup.com/mnras/article-lookup/doi/10.1046/j.1365-8711.2003.06486.x | |
dc.rights | © 2003, Royal Astronomical Society | en |
dc.subject | Accretion | en |
dc.subject | Accretion discs | en |
dc.subject | Close | en |
dc.subject | Stars | en |
dc.subject | Individual | en |
dc.subject | AC211 | en |
dc.subject | X2127+119 | en |
dc.subject | X-rays | en |
dc.subject | Binaries | en |
dc.title | Time-resolved spectroscopy of the M15 X-ray binary AC211/X2127+119 | en |
dc.type | Article (peer-reviewed) | en |
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