A strong emission line near 24.8 angstrom in the X-ray binary system MAXI J0556--332: gravitational...
A strong emission line near 24.8 angstrom in the X-ray binary system MAXI J0556--332: gravitational redshift or unusual donor?
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We report the discovery of a strong emission line near 24.8 angstrom (0.5 keV) in the newly discovered X-ray binary system MAXI J0556-332 with the reflection grating spectrometer onboard the XMM-Newton observatory. The X-ray light curve morphology during these observations is complex and shows occasional dipping behavior. Here we present time- and...
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A strong emission line near 24.8 angstrom in the X-ray binary system MAXI J0556--332: gravitational redshift or unusual donor?
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TN_cdi_proquest_journals_2082214641
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082214641
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2331-8422
DOI
10.48550/arxiv.1110.6918
