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dc.contributor.author Prabhu, T. P
dc.date.accessioned 2008-12-17T12:23:10Z
dc.date.available 2008-12-17T12:23:10Z
dc.date.issued 1980-04
dc.identifier.citation Astrophysics and Space Science, Vol. 68, No. 2, pp. 519 - 523 en
dc.identifier.issn 0004-640X
dc.identifier.uri http://hdl.handle.net/2248/4092
dc.description Open Access
dc.description.abstract The 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.iso en en
dc.publisher D.Reidel Publishing Co., en
dc.relation.uri http://adsabs.harvard.edu/abs/1980Ap%26SS..68..519P en
dc.relation.uri http://dx.doi.org/10.1007/BF00639719 en
dc.rights ©D.Reidel Publishing Co.,
dc.subject Astronomical Photography en
dc.subject Galactic Nuclei en
dc.subject Infrared Photography en
dc.subject Spiral Galaxies en
dc.subject Milky Way Galaxy en
dc.subject Near Infrared Radiation en
dc.subject Seyfert Galaxies en
dc.title Nucleus of NGC 2903 en
dc.type Article en


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