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2012MNRAS.424.2265L - Mon. Not. R. Astron. Soc., 424, 2265-2275 (2012/August-2)
Population synthesis for symbiotic X-ray binaries.
LU G.-L., ZHU C.-H., POSTNOV K.A., YUNGELSON L.R., KURANOV A.G. and WANG N.
Abstract (from CDS):
Among known SyXBs or candidate systems, 4U 1954+31 and IGR J16358-4724 in which the NSs have very long spin periods may host quasi-spherically accreting NSs. GX 1+4 has a peculiar long-term spin behaviour and it may also be a quasi-spherical wind-accreting source. We cannot identify whether there are wind-fed accretion discs in 4U 1700+24, Sct X-1, IRXS J180431.1-273932 and 2XMM J174016.0-290337. A search of CO emission lines in blazars: the low molecular gas content of BL Lac objects compared to quasars
Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society 2012 RAS
Journal keyword(s): binaries: symbiotic - stars: neutron - X-rays: stars of China (NSFC) Knowledge Innovation Program of the Chinese Academy of Sciences KJCX2-YW-T09 of China Natural Science Foundation of Xinjiang 2010211B05 University 10-02-00951
Simbad objects: 14
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