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arXiv · astro-ph/0612302

Discovery of a New X-Ray Burst/Millisecond Accreting Pulsar HETE J1900.1-2455

M. Suzuki·N. Kawai·T. Tamagawa·A. Yoshida·Y. E. Nakagawa·K. Tanaka·Y. Shirasaki·M. Matsuoka·G. R. Ricker·R. Vanderspek·N. Butler·D. Q. Lamb·C. Graziani·G. Pizzichini·R. Sato·M. Arimoto·J. Kotoku·M. Maetou·M. Yamauchi
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Abstract

A class of low-mass X-ray binary sources are known to be both X-ray burst sources and millisecond pulsars at the same time. A new source of this class was discovered by High Energy Transient Explorer 2 (HETE-2) on 14 June 2005 as a source of type-I X-ray bursts, which was named HETE J1900.1-2455. Five X-ray bursts from HETE J1900.1-2455 were observed during the summer of 2005. The time resolved spectral analysis of these bursts have revealed that their spectra are consistent with the blackbody radiation throughout the bursts. The bursts show the indication of radius expansion. The bolometric flux remains almost constant during the photospheric radius expansion while blackbody temperature dropped during the same period. Assuming that the flux reached to the Eddington limit on a standard 1.4 solar mass neutron star with a helium atmosphere, we estimate the distance to the source to be $\sim$ 4 kpc.

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M. Suzuki, N. Kawai, T. Tamagawa, A. Yoshida, Y. E. Nakagawa, K. Tanaka, Y. Shirasaki, M. Matsuoka, G. R. Ricker, R. Vanderspek, N. Butler, D. Q. Lamb, C. Graziani, G. Pizzichini, R. Sato, M. Arimoto, J. Kotoku, M. Maetou, M. Yamauchi. 2006-12-12. Discovery of a New X-Ray Burst/Millisecond Accreting Pulsar HETE J1900.1-2455. https://doi.org/10.1093/pasj%2F59.1.263

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