Observational study of core-collapse supernovae with diminishing hydrogen envelope

dc.contributor.author	Gangopadhyay, Anjasha
dc.date.accessioned	2021-03-26T06:33:43Z
dc.date.available	2021-03-26T06:33:43Z
dc.date.issued	2020-01
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/1272
dc.description	A thesis submitted to Pt. Ravishankar Shukla University, Raipur for the Degree of Doctor of Philosophy in Physics under the supervision of Dr. Kuntal Misra	en_US
dc.description.abstract	Supernovae (SNe) are the giant stellar explosions that brie y outshines the whole galaxy and enhances chemical enrichment. The thesis highlights a group of SNe with diminishing Hydrogen envelope. This mostly comprises of two groups - the stripped envelope group (SE-SNe, type IIb, Ib and Ic SNe) which strips o their outer envelopes due to high stellar winds or accretion with a nearby companion and the interacting SNe (type IIn, Ibn SNe) group which gains outer envelope due to interaction with a nearby circumstellar medium (CSM). In this thesis, we studied in depth the photometric and spectroscopic analysis of this group and derived a correlation between the members.	en_US
dc.description.sponsorship	ARIES, Nainital	en_US
dc.language.iso	en_US	en_US
dc.publisher	ARIES, Nainital	en_US
dc.relation.ispartofseries	Anjasha_thesis;
dc.subject	Supernovae; Photometric and spectroscopic;	en_US
dc.title	Observational study of core-collapse supernovae with diminishing hydrogen envelope	en_US
dc.type	Thesis	en_US