Central star formation in I Zw 81 : A massive S0 galaxy in the Bootes Void

Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/3752

Full metadata record

DC Field	Value	Language
dc.contributor.author	Ananta, C. Pradhan	-
dc.date.accessioned	2022-10-17T05:14:11Z	-
dc.date.available	2022-10-17T05:14:11Z	-
dc.date.issued	2022-09	-
dc.identifier.citation	Conference on "Celebraring seven years of Astrosat" ISRo, Bangalore, 28-29 Sept 2022	en_US
dc.identifier.uri	http://hdl.handle.net/2080/3752	-
dc.description	Copyright belongs to proceeding publisher	en_US
dc.description.abstract	Sparse environment of the void impacts the ongoing star formation in the galaxy. I Zw 81 is able to conserve its gas supply for a longer period of time due to lack of external perturbations.Star formation enhancement from minor-merger interaction is suspected.Low luminosity AGN is unable to quench the star formation in the galaxy. Central star formation is produced due to the action of bar. The bar tunnels gas from outskirts of the galaxy leaving a red outer disk.	en_US
dc.subject	void galaxies	en_US
dc.subject	Spectral energy distribution	en_US
dc.title	Central star formation in I Zw 81 : A massive S0 galaxy in the Bootes Void	en_US
Appears in Collections:	Conference Papers

Files in This Item:

File	Description	Size	Format
PradhanA_CSYA 2022.pdf		1.04 MB	Adobe PDF	View/Open