arXiv · 0709.4026
Recycling Matter in the Universe. X-ray observations of SBS 1150+599A (PN G135.9+55.9)
Abstract
We present X-ray observations of the close binary nucleus of the planetary nebula SBS 1150+599A obtained with the XMM-Newton satellite. Only one component of the binary can be observed in optical-UV. New X-ray observations show that the previously invisible component is a very hot compact star. This finding allows us to deduce rough values for the basic parameters of the binary. With a high probability the total mass of the system exceeds Chandrasekhar limit and makes the SBS 1150+599A one of the best candidate for a supernova type Ia progenitor.
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Gagik Tovmassian, John Tomsick, Ralf Napiwotzki, Lev Yungelson, Miriam Peña, Grazyna Stasińska, Michael Richer. 2007-09-25. Recycling Matter in the Universe. X-ray observations of SBS 1150+599A (PN G135.9+55.9). https://doi.org/10.1063/1.2840455
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