Domitilla de Martino
Istituto nazionale di astrofisica
13 papers found
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The C/N ratio from FUV spectroscopy as a constraint on evolution of the dwarf nova HS 0218 + 3229
UploadOptical and ultraviolet pulsed emission from an accreting millisecond pulsar
Download from www.nature.comGaia white dwarfs within 40 pc I: spectroscopic observations of new candidates
Download from academic.oup.comEvidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73–033933.0
UploadBroad-band characteristics of seven new hard X-ray selected cataclysmic variables
Download from repositorio.unab.clCXO J004318.8+412016, a steady supersoft X-ray source in M 31
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