Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/3745
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dc.contributor.authorPandey, Divya-
dc.contributor.authorSaha, Kanak-
dc.contributor.authorPradhan, Ananta C.-
dc.date.accessioned2022-09-16T07:07:13Z-
dc.date.available2022-09-16T07:07:13Z-
dc.date.issued2022-08-
dc.identifier.citationXXXIst International Astronomical Union General Assembly (IAUGA 2022), Busan, Republic of Korea August2-11, 2022en_US
dc.identifier.urihttp://hdl.handle.net/2080/3745-
dc.descriptionCopyright belongs to proceeding publisheren_US
dc.description.abstractWe study the multi-wavelength properties of a massive void galaxy - I Zw 81. The galaxy's structural decomposition reveals a strong bar at the center accompanied by a low surface brightness disk. The SED analysis of the galaxy indicate that the galaxy is star-forming. The central region of the galaxy comprising the bar shows signs of strong far- and near-UV emission while there is a dearth of recent star formation at the galactic outskirts. We comment on the role of bar and minor merger interaction in the evolution of I Zw 81.en_US
dc.subjectvoid galaxyen_US
dc.subjectevolution of I Zw 81en_US
dc.titleCentral star formation in I Zw 81 - Massive S0 galaxy in the Bootes Voiden_US
dc.typePresentationen_US
Appears in Collections:Conference Papers

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