The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations

The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations

<p>Abstract</p> <p>The aim of this paper is to give the radius of starlikeness of the certain classes of <inline-formula> <graphic file="1029-242X-2008-280183-i2.gif"/></inline-formula>-valent functions defined by multiplier transformations. The results...

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Main Authors: Polatog&#771;lu Ya&#351;ar, Yavuz Emel, Acu Mugur
Format: Article
Language:English
Published: SpringerOpen 2008-01-01
Series:Journal of Inequalities and Applications
Online Access:http://www.journalofinequalitiesandapplications.com/content/2008/280183
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spelling doaj-8eec4f460d1d4e39861b90c402103ef82020-11-25T00:17:33ZengSpringerOpenJournal of Inequalities and Applications1025-58341029-242X2008-01-0120081280183The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier TransformationsPolatog&#771;lu Ya&#351;arYavuz EmelAcu Mugur<p>Abstract</p> <p>The aim of this paper is to give the radius of starlikeness of the certain classes of <inline-formula> <graphic file="1029-242X-2008-280183-i2.gif"/></inline-formula>-valent functions defined by multiplier transformations. The results are obtained by using techniques of Robertson (1953,1963) which was used by Bernardi (1970), Libera (1971), Livingstone (1966), and Goel (1972). </p>http://www.journalofinequalitiesandapplications.com/content/2008/280183
collection DOAJ
language English
format Article
sources DOAJ
author Polatog&#771;lu Ya&#351;ar
Yavuz Emel
Acu Mugur
spellingShingle Polatog&#771;lu Ya&#351;ar
Yavuz Emel
Acu Mugur
The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
Journal of Inequalities and Applications
author_facet Polatog&#771;lu Ya&#351;ar
Yavuz Emel
Acu Mugur
author_sort Polatog&#771;lu Ya&#351;ar
title The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
title_short The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
title_full The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
title_fullStr The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
title_full_unstemmed The Radius of Starlikeness of the Certain Classes of <inline-formula> <graphic file="1029-242X-2008-280183-i1.gif"/></inline-formula>-Valent Functions Defined by Multiplier Transformations
title_sort radius of starlikeness of the certain classes of <inline-formula> <graphic file="1029-242x-2008-280183-i1.gif"/></inline-formula>-valent functions defined by multiplier transformations
publisher SpringerOpen
series Journal of Inequalities and Applications
issn 1025-5834
1029-242X
publishDate 2008-01-01
description <p>Abstract</p> <p>The aim of this paper is to give the radius of starlikeness of the certain classes of <inline-formula> <graphic file="1029-242X-2008-280183-i2.gif"/></inline-formula>-valent functions defined by multiplier transformations. The results are obtained by using techniques of Robertson (1953,1963) which was used by Bernardi (1970), Libera (1971), Livingstone (1966), and Goel (1972). </p>
url http://www.journalofinequalitiesandapplications.com/content/2008/280183
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