Yet another galaxy identification for an ultraluminous X-ray source (Articolo in rivista)

Type
Label
  • Yet another galaxy identification for an ultraluminous X-ray source (Articolo in rivista) (literal)
Anno
  • 2003-01-01T00:00:00+01:00 (literal)
Alternative label
  • Masetti N., L. Foschini, L.C. Ho, M. Dadina, G. Di Cocco, G. Malaguti, E. Palazzi (2003)
    Yet another galaxy identification for an ultraluminous X-ray source
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Masetti N., L. Foschini, L.C. Ho, M. Dadina, G. Di Cocco, G. Malaguti, E. Palazzi (literal)
Pagina inizio
  • L27 (literal)
Pagina fine
  • L32 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 406 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Titolo
  • Yet another galaxy identification for an ultraluminous X-ray source (literal)
Abstract
  • We report on the identification of the optical and infrared counterparts of the ultraluminous X-ray source (ULX) XMMU J121214.5+131248 (NGC4168-ULX1). The optical spectrum yields a redshift of z=0.217, which implies that the ULX is not associated with the nearby galaxy NGC 4168, but rather with a background object. Optical spectral line ratios and the spectral energy distribution constructed from the available data indicate that the source is likely a starburst nucleus. (literal)
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