in this paper, we give some characterizations for legendre spherical, legendre normal and legendre rectifying curves in the 3-dimensional sasakian space. furthermore, we show that legendre spherical curves are also legendre normal curves. in particular, we prove that the inverse of curvature of a legendre rectifying curve is a non-constant linear function of the arclength parameter.

Recently. ic-X analysis with the “D” value was developed by Ault to detect a minor population of malignant B cells in peripheral blood. This analysis is based on the KolmogorovSmirnov test, and the D value is calculated by a flowcytometer and a computer. We have recently devised a more sensitive parameter for the sc-X analysis than the D value called the .-curve (&c); the #{244}c applies the sa...

background: the aim of this research was to determine and compare emotional quotient and clinical performance in type d and non-d personality anesthesiology residents. methods: this was a causative–comparative research consenting anesthesiology residents (n=48). all the participants completed bar-on emotional quotient and ds-14 (type d personality) questionnaires. clinical performance of partic...

Let a be an ideal of holomorphic functions vanishing only at the origin in C. The type of a is an invariant that measures the order of vanishing of the functions in a along holomorphic curves; this invariant is of importance in the study of subelliptic estimates and subelliptic multiplier ideal sheaves. Recently there has been some interest in the question of which curves actually compute the t...

In this study, to know about the phylogeny of Escherichia coli isolated from broilers with collibacillosis in Tabriz, 70 E. coli isolates recovered from broilers with collibacillosis were characterized for phylogenetic group (A, B1, B2, D) by multiplex PCR. Of the all 70 samples, 35 (50%) isolates were classified as type A, 32 (45%) as type D, 2 (2.8%) as type B1 and 1 (2.8%) as type B2. This s...

ABSTRACT We present optical spectroscopy together with ultraviolet, optical, and near-infrared photometry of SN 2019hcc, which resides in a host galaxy at redshift 0.044, displaying sub-solar metallicity. The supernova spectrum near peak epoch shows ‘w’ shape around 4000 Å is usually associated O ii lines typical Type I superluminous supernovae. 2019hcc post-peak spectra show well-developed H ?...