1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2160
Full metadata record
DC FieldValueLanguage
dc.contributor.authorNamboodiri, P. M. S-
dc.date.accessioned2008-03-15T11:15:51Z-
dc.date.available2008-03-15T11:15:51Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 397 - 399en
dc.identifier.urihttp://hdl.handle.net/2248/2160-
dc.description.abstractNumerical simulations of equal mass galaxies, moving initially on a parabolic orbit, have been performed to see how the total energy of the system changes in close and wide encounters. The results are compared with those obtained using impulse approximation.en
dc.format.extent146395 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..397Nen
dc.subjectGalaxiesen
dc.subjectInteractionsen
dc.subjectNumerical simulationsen
dc.titleTidal interactions in spherical galaxiesen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
pms.pdf142.96 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.