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DC Field | Value | Language |
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dc.contributor.advisor | Nath, Biman | - |
dc.contributor.author | Jana, Ranita | - |
dc.date.accessioned | 2022-07-18T06:17:26Z | - |
dc.date.available | 2022-07-18T06:17:26Z | - |
dc.date.issued | 2022-04-21 | - |
dc.identifier.citation | Ph.D. Thesis, Jawaharlal Nehru University, New Delhi, 2022 | en_US |
dc.identifier.uri | http://hdl.handle.net/2289/7975 | - |
dc.description | Restricted Access | en_US |
dc.description.abstract | Galaxies are the largest gravitationally bound structures in the Universe that can form stars. The morphology and star formation rate of the galaxies evolve with time. They interact with each other through merger events. They also interact with the surrounding diffuse gaseous medium in a number of ways. Both these interactions play an important role in the evolution of galaxies. The aim of this thesis is to study the interaction between galaxies and their surrounding medium. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Raman Research Institute, Benglauru | en_US |
dc.rights | This thesis is posted here with the permission of the author. Personal use of this material is permitted. Any other use requires prior permission of the author. By choosing to view this document, you agree to all provisions of the copyright laws protecting it. | en_US |
dc.subject.classification | Astronomy and Astrophysics | en |
dc.title | Interaction of galaxies and thier surroundings through cosmic rays | en_US |
dc.type | Thesis | en_US |
Appears in Collections: | Theses (A&A) |
Files in This Item:
File | Description | Size | Format | |
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Thesis_Ranita_final(1).pdf Restricted Access | Restricted Access | 16.67 MB | Adobe PDF | View/Open Request a copy |
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