Thermal Featureless Spectrum: Evidence for Bare Strange Stars

Details Thermal Featureless Spectrum: Evidence for Bare Strange Stars Thermal Featureless Spectrum: Evidence for Bare Strange Stars

2002-02-20

arxiv.org/abs/astro-ph/0202365v2

Astrophys.J. 570 (2002) L65-L68

Astronomy and Astrophysics

Astrophysics

4 pages, revised version to be published in ApJL, or at http://vega.bac.pku.edu.cn/~rxxu/publications/index_P.htm

Scientific paper

10.1086/340993

Motivated by trying to understand the absence of spectral lines in the thermal components of the X-ray compact sources observed recently by Chandra or XMM, we propose that these sources could be simply bare strange stars. The formation, cooling, and thermal photon radiation of bare strange stars have been investigated. It is suggested that thermal featureless spectrum could be a new probe for identifying strange stars.

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