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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1880
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dc.contributor.authorBhatt, H. C-
dc.date.accessioned2007-10-11T12:10:15Z-
dc.date.available2007-10-11T12:10:15Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 51 - 59en
dc.identifier.urihttp://hdl.handle.net/2248/1880-
dc.description.abstractRecent discoveries of substellar and planetary-mass objects in orbit around other stars represent the most remarkable progress achieved in the search for extrasolar planetary systems. The evidence for their existence is summarised. The physical properties and orbital characteristics of these systems are discussed and compared with those of the solar system. The new discoveries raise new questions for the theories of planet formation as part of the star formation process.en
dc.format.extent886535 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27...51Ben
dc.subjectSun-like starsen
dc.subjectExtrasolar planetsen
dc.subjectStar formationen
dc.subjectPlanet formationen
dc.titlePlanet formation in sun-like systemsen
dc.typeArticleen
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