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Issue A&A
Volume 399, Number 2, February IV 2003
Page(s) 663 - 680
Section Stellar atmospheres
DOI http://dx.doi.org/10.1051/0004-6361:20021781



A&A 399, 663-680 (2003)
DOI: 10.1051/0004-6361:20021781

Photospheric radius expansion X-ray bursts as standard candles

E. Kuulkers1, 2, P. R. den Hartog1, 2, J. J. M. in 't Zand1, F. W. M. Verbunt2, W. E. Harris3 and M. Cocchi4

1  SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
    e-mail: Erik.Kuulkers@rssd.esa.int
2  Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands
3  Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada
4  Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF) Area Ricerca Roma Tor Vergata, Via del Fosso del Cavaliere, 00133 Roma, Italy

(Received 21 May 2002 / Accepted 29 November 2002 )

Abstract
We examined the maximum bolometric peak luminosities during type I X-ray bursts from the persistent or transient luminous X-ray sources in globular clusters. We show that for about two thirds of the sources the maximum peak luminosities during photospheric radius expansion X-ray bursts extend to a critical value of $3.79 \pm 0.15 \times 10 ^{38}$ erg s -1, assuming the total X-ray burst emission is entirely due to black-body radiation and the recorded maximum luminosity is the actual peak luminosity. This empirical critical luminosity is consistent with the Eddington luminosity limit for hydrogen poor material. Since the critical luminosity is more or less always reached during photospheric radius expansion X-ray bursts (except for one source), such bursts may be regarded as empirical standard candles. However, because significant deviations do occur, our standard candle is only accurate to within 15%. We re-evaluated the distances to the twelve globular clusters in which the X-ray bursters reside.


Key words: binaries: close -- stars: neutron -- globular clusters: general -- X-rays: binaries -- X-rays: bursts

Offprint request: E. Kuulkers, ekuulker@rssd.esa.int

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