A Class of Harmonic Starlike Functions with Respect to Symmetric Points Associated with Wright Generalized Hypergeometric Function
Anal. Theory Appl., 28 (2012), pp. 363-376.
Published online: 2012-12
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@Article{ATA-28-363,
author = {M. K. Aouf, R. M. El-Ashwah, A. Shamandy and S. M. El-Deeb},
title = {A Class of Harmonic Starlike Functions with Respect to Symmetric Points Associated with Wright Generalized Hypergeometric Function},
journal = {Analysis in Theory and Applications},
year = {2012},
volume = {28},
number = {4},
pages = {363--376},
abstract = {
Making use of Wright operator we introduce a new class of complex-valued harmonic functions with respect to symmetric points which are orientation preserving, univalent and starlike. We obtain coefficient conditions, extreme points, distortion bounds, and convex combination.
}, issn = {1573-8175}, doi = {https://doi.org/10.3969/j.issn.1672-4070.2012.04.005}, url = {http://global-sci.org/intro/article_detail/ata/4570.html} }
TY - JOUR
T1 - A Class of Harmonic Starlike Functions with Respect to Symmetric Points Associated with Wright Generalized Hypergeometric Function
AU - M. K. Aouf, R. M. El-Ashwah, A. Shamandy & S. M. El-Deeb
JO - Analysis in Theory and Applications
VL - 4
SP - 363
EP - 376
PY - 2012
DA - 2012/12
SN - 28
DO - http://doi.org/10.3969/j.issn.1672-4070.2012.04.005
UR - https://global-sci.org/intro/article_detail/ata/4570.html
KW - harmonic, univalent, Wright operator, symmetric point.
AB -
Making use of Wright operator we introduce a new class of complex-valued harmonic functions with respect to symmetric points which are orientation preserving, univalent and starlike. We obtain coefficient conditions, extreme points, distortion bounds, and convex combination.
M. K. Aouf, R. M. El-Ashwah, A. Shamandy and S. M. El-Deeb. (2012). A Class of Harmonic Starlike Functions with Respect to Symmetric Points Associated with Wright Generalized Hypergeometric Function.
Analysis in Theory and Applications. 28 (4).
363-376.
doi:10.3969/j.issn.1672-4070.2012.04.005
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