نتایج جستجو برای: stars

تعداد نتایج: 56510  

In this paper, the concept of incidence domination number of graphs  is introduced and the incidence dominating set and  the incidence domination number  of some particular graphs such as  paths, cycles, wheels, complete graphs and stars are studied.

پایان نامه :وزارت علوم، تحقیقات و فناوری - دانشگاه سیستان و بلوچستان - دانشکده مهندسی عمران 1393

پیش بینی خصوصیات جریان در رودخانه ها از نیاز های اساسی در طرح¬های مهندسی رودخانه است. با این وجود باید بتوان با داشتن اطلاعاتی از مورفولوژی رودخانه¬ها به پیش¬بینی¬های هیدرولیکی قابل قبولی دست یافت. امروزه مدل¬های ریاضی می¬توانند با گرفتن اطلاعات از هندسه محل عبور جریان و رسوب عبوری از آن و همچنین با داشتن اطلاعات هیدرولیکی، روندیابی آب و رسوب را به منظور تحلیل مسائل پیچیده مهندسی رودخانه انجام ...

We have studied the effect of hypothetical Cosmions on the core stability of main sequence stars (of populations I and II). Cosmions, with a mass of 4-10 Gev/c2 and a scattering cross section with nucleons of approximately 10-36 cm2 could prevail in transporting heat in the stellar cores. Raby [17] showed the existence of a local thermal instability caused by the presence of Cosmions in the sol...

Journal: :journal of sciences islamic republic of iran 0
m.y. rahimi ardabili department of applied mathematics, faculty of mathematics, tabriz university, tabriz, islamic republic of iran

the linear adiabatic pulsation-periods of mira variable stars have been derived. approximately 2701[1]models were calculated for m = 0.7 mθ to 2 mθ stars with radii from 180 rθ to 340 rθ and luminosities from 2800 lθ to 10,000 lθ. the chemical composition of all models is (x,z) = (0.7,0.02). from the result of this study, linear relations on luminosity-period-mass relationship and luminosity-pe...

Journal: :journal of sciences islamic republic of iran 0

we have studied the effect of hypothetical cosmions on the core stability of main sequence stars (of populations i and ii). cosmions, with a mass of 4-10 gev/c2 and a scattering cross section with nucleons of approximately 10-36 cm2 could prevail in transporting heat in the stellar cores. raby [17] showed the existence of a local thermal instability caused by the presence of cosmions in the sol...

Journal: :iranian journal of optimization 0
jafar fathali department of mathematics, shahrood university of technology, university blvd., shahrood, iran nader jafari rad department of mathematics, shahrood university of technology, university blvd., shahrood, iran sadegh rahimi sherbaf department of mathematics, shahrood university of technology, university blvd., shahrood, iran

an extended star is a tree which has only one vertex with degree larger than two. the -center problem in a graph  asks to find a subset  of the vertices of  of cardinality  such that the maximum weighted distances from  to all vertices is minimized. in this paper we consider the -center problem on the unweighted extended stars, and present some properties to find solution.

Our galaxy is a spiral galaxy and its stars are mostly in a thin disk and rotate around the galactic center. The vertical component of the dispersion velocity of stars is a function of the galactic latitude and decreases with increasing it. In the galactic Besancon model, this dependence is ignored and they just consider the dependence of dispersion velocity on the stellar age. Becanson model i...

ژورنال: پژوهش های ریاضی 2019

Introduction This paper presents an algorithm for covering orthogonal polygons with minimal number of guards. This idea examines the minimum number of guards for orthogonal simple polygons (without holes) for all scenarios and can also find a rectangular area for each guards. We consider the problem of covering orthogonal polygons with a minimum number of r-stars. In each orthogonal polygon P,...

Journal: رستنیها 2012

Fungi belonging to the genus Geastrum are known as earth stars due to different layers with specific alignment in fruit-bodies. In this paper four species of the genus Geastrum viz. G. coronatum, G. rufescens, G. saccatum and G. schmidelii were reported as new for Iran. Previously reported specimen, G. corollinum (as G. recolligens)was newly collected and was studied in details. Newly reported ...

The sum of distances between all the pairs of vertices in a connected graph is known as the {it Wiener index} of the graph. In this paper, we obtain the Wiener index of edge complements of stars, complete subgraphs and cycles in $K_n$.

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