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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4092
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dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-12-17T12:23:10Z-
dc.date.available2008-12-17T12:23:10Z-
dc.date.issued1980-04-
dc.identifier.citationAstrophysics and Space Science, Vol. 68, No. 2, pp. 519 - 523en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4092-
dc.descriptionOpen Access-
dc.description.abstractThe nucleus of NGC 2903 is identified on near infrared photographs. The energy distribution of this nucleus in the visual region of the spectrum is estimated from available observations. The continuum compares well with the nuclei of Seyfert galaxies, but is weaker by one to two orders of magnitude.en
dc.language.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://adsabs.harvard.edu/abs/1980Ap%26SS..68..519Pen
dc.relation.urihttp://dx.doi.org/10.1007/BF00639719en
dc.rights©D.Reidel Publishing Co.,-
dc.subjectAstronomical Photographyen
dc.subjectGalactic Nucleien
dc.subjectInfrared Photographyen
dc.subjectSpiral Galaxiesen
dc.subjectMilky Way Galaxyen
dc.subjectNear Infrared Radiationen
dc.subjectSeyfert Galaxiesen
dc.titleNucleus of NGC 2903en
dc.typeArticleen
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