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dc.contributor.authorStrauss, Federico Maximopt_BR
dc.date.accessioned2014-07-23T02:04:38Zpt_BR
dc.date.issued1977pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98388pt_BR
dc.description.abstractA high signal to noise ratio and good one dimensional resolution are obtained by scanning a narrow slit across extended objects. Several observations of two comets give information on total brightness and on the density distribution of the coma. The characteristic scale length reduced to 1 AU of the coma of comet Bradfield was 10⁴·⁸±⁰·¹ km, in agreement with that of C₂ in comet Bennet (1970 II) obtained by Delsemme and Moreau (1973). For comet Kohoutek we obtained a slightly larger value, 10⁵·⁰±⁰·¹ km.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. Berlin. Vol. 55, no. 2 (Mar. 1977), p. 299-302pt_BR
dc.rightsOpen Accessen
dc.subjectPhotometryen
dc.subjectCometaspt_BR
dc.subjectAstrofisica do sistema solarpt_BR
dc.subjectCometsen
dc.titleStrip photometry of diffuse objects : i. the structure of comets kohoutek (1973 xii) and bradfield (1974 iii)pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000146224pt_BR
dc.type.originEstrangeiropt_BR


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