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pro vyhledávání: '"Edwards, Z. I."'
Autor:
Seward, F. D., Charles, P. A., Foster, D. L., Dickel, J. R., Romero, P. S., Edwards, Z. I., Perry, M., Williams, R. M.
A Chandra observation of the Large Magellanic Cloud supernova remnant DEM L241 reveals an interior unresolved source which is probably an accretion-powered binary. The optical counterpart is an O5III(f) star making this a High-Mass X-ray Binary (HMXB
Externí odkaz:
http://arxiv.org/abs/1208.1453
