Star formation - Open Access .click

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1974
Before discussing problems of star formation and star destruction it will be as well to describe some of the more important features of stellar evolution. We begin at a very early stage, when an object has recognisably become a star. This means that the object is opaque and violent mass motions have ceased.
openaire +2 more sources

The Formation of Star Clusters

American Scientist, 1998
Bruce G. Elmegreen, Yuri N. Efremov
openaire +2 more sources

Coalescence of black hole–neutron star binaries

Living Reviews in Relativity, 2021
Koutarou Kyutoku, Masaru Shibata, Keisuke Taniguchi +2 more
exaly

Star Formation

The Moon and the Planets, 1980
openaire +1 more source

Constraining neutron-star matter with microscopic and macroscopic collisions

Nature, 2022
Sabrina Huth, Peter T H Pang, Ingo Tews
exaly

Star Polymers

Chemical Reviews, 2016
Jing M Ren, Thomas G Mckenzie
exaly

Neutron star mergers and how to study them

Living Reviews in Relativity, 2020
Eric Burns
exaly