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Issue A&A
Volume 392, Number 3, September IV 2002
Page(s) 931 - 936
Section Formation, structure and evolution of stars
DOI http://dx.doi.org/10.1051/0004-6361:20021183



A&A 392, 931-936 (2002)
DOI: 10.1051/0004-6361:20021183

Chandra follow-up of bursters with low persistent emission

R. Cornelisse1, 2, F. Verbunt2, J. J. M. in 't Zand2, 1, E. Kuulkers1, 2 and J. Heise1

1  SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
2  Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands

( Received 13 February 2002 / Accepted 21 June 2002 )

Abstract
We report on Chandra ACIS-S observations of five type I X-ray bursters with low persistent emission: SAX J1324.5-6313, SAX J1752.3-3128, SAX J1753.5-2349, SAX J1806.5-2215, and SAX J1818.7+1424. We designate candidate persistent sources for four X-ray bursters. All candidates are detected at a persistent luminosity level of 10 $^{32-33}~{\rm erg\,s}^{-1}$, comparable to soft X-ray transients in quiescence. From the number of bursters with low persistent emission detected so far with the Wide Field Cameras, we estimate a total of such sources in our Galaxy between 30 and 4000.


Key words: binaries: close -- stars: individual: SAX J1324.5-6313, SAX J1752.3-3128, SAX J1753.5-2349, SAX J1806.5-2215, SAX J1818.7+1424  -- stars: neutron -- X-rays: bursts

Offprint request: R. Cornelisse, R.Cornelisse@sron.nl

SIMBAD Objects in preparation



© ESO 2002


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