Theory of the continuous spectrum of gaseous nebula of pure hydrogen

dc.creatorGerola, H.
dc.creatorPanagia, N.
dc.date1970
dc.date2020-06-09T14:38:25Z
dc.date.accessioned2023-07-14T20:45:09Z
dc.date.available2023-07-14T20:45:09Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/97840
dc.identifierissn:1669-9521
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7440458
dc.descriptionIt has been studied the formation of the continuum of nebular hydrogen when ionization is due to radiation and to collisions. Two photon emission and continuous emissivity in the reaction of formation of H- have been included. The continuum results extremely sensitive to the relative amount of the two types of thermal excitation.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectGalaxias
dc.titleTheory of the continuous spectrum of gaseous nebula of pure hydrogen
dc.typeArticulo
dc.typeComunicacion


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