The first generation of stars formation at Redshift Z=0 and when did they lit up the dark matter?

Rupak Bhattacharya; Dr.Pranab Kumar Bhattacharya; Upasana Bhattacharya; Ritwik Bhattacharya; Aiyshi Mukherjee; Rupsha Bhattacharya; Debasish Mukherjee; Dalia Mukherjee; Hindol Banerjee

Abstract

Our home is our own life galaxy, the "Milky Way” which consist of trillions and trillions of stars. One of the middle aged, yellow stars is our sun. 400 billions of stars moving with a very complex and orderly grace in our spiral galaxy the Milky Way. In all galaxies there are perhaps as many as many planets as stars i.e 1011 × 1011 =1022, 10 billion trillions planets. Some stars are solitary (though in a binary star formation system) like our sun and most of the stars have their own companions. Systems of stars are commonly seen double, i.e two stars are orbiting one another. Some stars are so close that they touch each other and star staff flow beneath them. Most stars are however separated from one another by vast space-time. Stars are born and they dies too. Some stars went into novas and or in supernovas and are as bright as the entire galaxy that contains them. Some stars end them in black holes and are invisible even from a few hundred kilometers away. Some stars are in triple star systems, some are in binary star systems. Some stars are blue hot and very young. Some stars are yellow stars. Yellow stars are conventionally middle aged, while red (red giants) stars are elderly or dyeing stars. Some stars are in white dwarfs and they are in the final stage of death. Our '' sun” is a second generation star of a binary star formation process, produced by collapse of gases, Interstellar clouds within the framework of spiral pattern, a gaseous cloud which contains material required for nuclear furnaces, appearing inside the star. Stars are formed of giant interstellar mass, molecular clouds, containing trillions and trillions tons of gaseous hydrogen and deuterium ions as they collapse under gravity. Now in the dense clouds containing perhaps ten thousands millions (1010) atoms per cubic centimetre- that represent a much more dense collection of material, rather than gaseous material in stars, how are they converted into bright stars? How the stars were formed in the nebula or in galaxies of the universe? Stars formation is an astronomical puzzle that involves pure poor understanding of how interstellar giant molecular clouds (CDM+HDM) turned into the stars! Stars are formed from protostellar condensation in the star forming regions like Nebulas.

Abstract

Keywords