Mass Function of Young and Embedded Star Clusters

dc.contributor.guide	Routh, Swati and Sujatha, S
dc.coverage.spatial
dc.creator.researcher	Krishna Kumar Kowshik
dc.date.accessioned	2024-10-01T06:59:39Z
dc.date.available	2024-10-01T06:59:39Z
dc.date.awarded	2023
dc.date.completed	2024
dc.date.registered
dc.description.abstract	Our galaxy has nearly 1011 stars and nearly all of them are located in the galactic disc. Within the disc structure, several clusters and associations of stars are found. They are gravitationally bound systems of stars which are born in the same region of space from a single molecular cloud and are often regarded as a basic unit of star formation. Therefore, due to their similar distances, coevality, chemical compositions, luminosities, and stellar masses, the study of star clusters is advantageous. newline
dc.description.note
dc.format.accompanyingmaterial	None
dc.format.dimensions
dc.format.extent
dc.identifier.uri	http://hdl.handle.net/10603/592942
dc.language	English
dc.publisher.institution	Physics
dc.publisher.place	Bengaluru
dc.publisher.university	Jain University
dc.relation
dc.rights	university
dc.source.university	University
dc.subject.keyword	Physical Sciences
dc.subject.keyword	Physics
dc.subject.keyword	Physics Particles and Fields
dc.title	Mass Function of Young and Embedded Star Clusters
dc.title.alternative
dc.type.degree	Ph.D.