Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4123
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dc.contributor.authorBabu, G. S. D-
dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-12-18T14:47:17Z-
dc.date.available2008-12-18T14:47:17Z-
dc.date.issued1981-09-
dc.identifier.citationAstrophysics and Space Science, Vol. 79, No. 1, pp. 243 - 255en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4123-
dc.description.abstractThe physical parameters, such as the effective temperatures, radii, bolometric magnitudes and bolometric corrections of 87 Ap and Am stars out of the 125 compiled here are essentially based on the work done by the authors at the Kavalur Observatory. The results of the rest of the stars are from the earlier work done by one of the authors, which have been included for the sake of completion. All the results are derived from the observed energy distribution curves of the individual stars. The standardised magnitudes at various wavelengths also have been listeden
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1981Ap%26SS..79..243Ben
dc.relation.urihttp://dx.doi.org/10.1007/BF00655921en
dc.subjectA Starsen
dc.subjectAstrophysicsen
dc.subjectSpectral Energy Distributionen
dc.subjectStellar Magnitudeen
dc.subjectStellar Spectraen
dc.subjectStellar Temperatureen
dc.subjectAstrometryen
dc.subjectAstronomical Catalogsen
dc.subjectRadiien
dc.subjectStellar Spectrophotometryen
dc.titleA compilation of physical parameters of AP and AM stars as derived from energy distribution studiesen
dc.typeArticleen
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