Publication:
Distortion estimate and radius of starlikeness for generalized p-valent close-to-star functions

dc.contributorFen Edebiyat Fakültesi / Faculty of Letters and Sciences Matematik - Bilgisayar / Mathematics and Computer Sciencetr_TR
dc.contributor.authorÖzkan, H. Esra
dc.contributor.authorYavuz Duman, Emel
dc.contributor.authorID111202tr_TR
dc.date.accessioned2018-09-06T08:01:42Z
dc.date.available2018-09-06T08:01:42Z
dc.date.issued2013
dc.description.abstractLet A(p, n), n ≥ 1, p ≥ 1 be the class of all analytic functions in the open unit disc D = {z| |z| < 1} of the form f(z) = zp + anp+1znp+1 + anp+2znp+2 + ··· . Let g(z) be an element of A(p, n) such that g(z) satisfies the condition Re z g (z) g(z) > 0 for all z ∈ D, we then call g(z) the generalized p−valent starlike function in D. The class of such functions is denoted by S∗(p, n). Let s(z) be an element of A(p, n) and g(z) be an element of S∗(p, n). If the condition Re s(z) g(z) > 0 (z ∈ D), is satisfied then s(z) is called the generalized p−valent close-to-star function in D. The class of such functions is denoted by S∗K(p, n). The aim of this paper is to give a distortion estimation and the radius of starlikeness of the class S∗K(p, n).tr_TR
dc.identifier7tr_TR
dc.identifier7tr_TR
dc.identifier7tr_TR
dc.identifier.scopus2-s2.0-84874779180
dc.identifier.urihttps://hdl.handle.net/11413/2664
dc.language.isoen
dc.publisherHIKARI
dc.relationInt. J. Math. Anal.tr_TR
dc.subjectClose-to-star functiontr_TR
dc.subjectthe radius of starlikenesstr_TR
dc.subjectdistortion estimatetr_TR
dc.titleDistortion estimate and radius of starlikeness for generalized p-valent close-to-star functionstr_TR
dc.typeArticle
dspace.entity.typePublication
local.indexed.atScopus

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