Titlebook: Neutrosophic Operational Research; Methods and Applicat Florentin Smarandache,Mohamed Abdel-Basset Book 2021 The Editor(s) (if applicable)

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Truong Thi Thuy Duong,Nguyen Xuan Thao,Florentin Smarandachenomy, related space sciences and other related fields. This invaluable reference source (and its companion volume, .StarBriefs. .Plus.) should be on the reference shelf of every library, organization or individual with any interest in these areas. .The coverage includes relevant universities, scient

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不如樂死去

?erif ?zlü,?rfan Deli?s beginner-friendly scientific explanations behind every sto.Unbeknownst to many, our modern language contains countless words that were inspired by human observations of the cosmos. We now use words like “zenith”, “Monday”, “disaster”, “dog days”, “starfish”, “l(fā)unatic”, flu, and so many others, wit

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Faruk Karaaslan,Khizar Hayat,Chiranjibe Janaonal rate of 100–1000 M./year, there exists a much broader class of “normal” galaxies at z = 0 which do form stars at rates ranging from 0 (E+S0) to 10 M./year (BCDs), with the vast majority of normal disk galaxies doing it at 1 M./year. Much of what is known about the star formation properties of n

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Rehan Ahmad Khan Sherwani,Muhammad Aslam,Muhammad Ali Raza,Muhammad Farooq,Muhammad Abid,Muhammad Tag photons in a population of some age and metallicity, through the creation rate of various chemical elements, to the mass to light ratio of a system. This significance, together with the empirical difficulty to determine the IMF robustly, and the near complete lack of any robust theoretical predict

CLASH

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Mohamed Abdel-Basset,Mai Mohamed,Jun Yeonal rate of 100–1000 M./year, there exists a much broader class of “normal” galaxies at z = 0 which do form stars at rates ranging from 0 (E+S0) to 10 M./year (BCDs), with the vast majority of normal disk galaxies doing it at 1 M./year. Much of what is known about the star formation properties of n

逗它小傻瓜

Sahidul Islam I begin by defining starbursts in several different ways, and discuss the merits and limitations of these definitions. I will argue that the most physically useful definition of a starburst is its “intensity” (star-formation rate per unit area). This is the most natural parameter to compare local s