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A study on the formation of field, binary or multiple stars: a 2D approach through dynamical system
A. Mondal, , A. Sen
Published in Springer Science and Business Media B.V.
Volume: 366
Issue: 2
A dynamical model has been developed to envisage the star formation scenario in filamentary molecular clouds. In the present work a double well potential has been considered to find the number of stable stationary points as the origin of field star, binary stars or stellar associations. It is found that low density structure can lead to the formation of field stars while an intermediate density structure is favourable for formation of binary stars. Stellar associations are generally prevalent in dense filamentary molecular clouds. © 2021, The Author(s), under exclusive licence to Springer Nature B.V. part of Springer Nature.
About the journal
JournalData powered by TypesetAstrophysics and Space Science
PublisherData powered by TypesetSpringer Science and Business Media B.V.