Binary orbits as the driver of γ-ray emission and mass ejection in classical novae

From National Research Council Canada

DOIResolve DOI: https://doi.org/10.1038/nature13773
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Affiliation
  1. National Research Council of Canada. National Science Infrastructure
FormatText, Article
Subjectastrophysics; explosion; velocity; wavelength; X-ray spectroscopy; acceleration; gamma radiation; image analysis; motion; optical resolution; spectrum; synchrotron radiation; wind
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LanguageEnglish
Peer reviewedYes
NPARC number21272652
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Record identifier4fe775af-eaf9-49da-9e4b-371435b2b14a
Record created2014-12-03
Record modified2020-04-22
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