Timing of the 2008 outburst of SAX J1808.4–3658 with XMM-Newton:a stable orbital-period derivative over ten years

E-ISSN： 1432-0746|496|2|L17-L20

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.496, Iss.2, 2009-03, pp. : L17-L20

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

XMM-Newton detects a relativistically broadened iron line in the spectrum of the ms X-ray pulsar SAX J1808.4-3658

Astronomy & Astrophysics, Vol. 493, Iss. 3, 2009-01 ,pp. : L39-L43

Edp Sciences

Access to resources Recommend Favorite

New ephemeris of the ADC source 2A 1822–371:a stable orbital-period derivative over 30 years

By Burderi L. Di Salvo T. Riggio A. Papitto A. Iaria R. D'Aì A. Menna M. T.

Astronomy & Astrophysics, Vol. 515, Iss. issue, 2010-06 ,pp. : A44-A44

Edp Sciences

Access to resources Recommend Favorite

The first outburst of SAX J1808.4-3658 revisited

Astronomy & Astrophysics, Vol. 372, Iss. 3, 2001-06 ,pp. : 916-921

Edp Sciences

Access to resources Recommend Favorite

Phase-resolved spectroscopy of the accreting millisecond X-ray pulsar SAX J1808.4-3658 during the 2008 outburst

Astronomy & Astrophysics, Vol. 495, Iss. 1, 2009-02 ,pp. : L1-L4

Edp Sciences

Access to resources Recommend Favorite

Unveiling the nature of the highly absorbed X-ray source SAX J1748.2-2808 with XMM-Newton

Astronomy & Astrophysics, Vol. 456, Iss. 1, 2006-09 ,pp. : 287-293

Edp Sciences

Access to resources Recommend Favorite