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. Cocchi41 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
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
SIMBAD Objects
© ESO 2003

BibSonomy
CiteUlike
Del.icio.us
Digg
Facebook
Mendeley
Twitter