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The beauty of resolution: The SN Ib factory NGC 2770 spatially resolved

Published online by Cambridge University Press:  09 February 2015

C. C. Thöne ,
L. Christensen ,
J. Gorosabel  and
A. de Ugarte Postigo
C. C. Thöne
Affiliation:
Instituto de Astrofísica de Andalucía, Glorieta de la Astronomía s/n, 18008 Granada, Spain. email: cthoene@iaa.es
L. Christensen
Affiliation:
Dark Cosmology Centre, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
J. Gorosabel
Affiliation:
Instituto de Astrofísica de Andalucía, Glorieta de la Astronomía s/n, 18008 Granada, Spain. email: cthoene@iaa.es Unidad Asociada Grupo Ciencias Planetarias UPV/EHU-IAA/CSIC, Departamento de Física Aplicada I, E.T.S., Ingeniería, Universidad del País Vasco UPV/EHU, E-48013 Bilbao, Spain Ikerbasque, Basque Foundation for Science, E-48008 Bilbao, Spain
A. de Ugarte Postigo
Affiliation:
Instituto de Astrofísica de Andalucía, Glorieta de la Astronomía s/n, 18008 Granada, Spain. email: cthoene@iaa.es Dark Cosmology Centre, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
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Abstract

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The late-type spiral NGC 2770 hosted 3 Type Ib supernovae (SNe) in or next to star-forming regions in its outer spiral arms. We study the properties of the SN sites and the galaxy at different spatial resolutions to infer propeties of the SN progenitors and the SF history of the galaxy. Several 3D techniques are used and, for the first time, we present images of metallicity, shocks and stellar population ages from OSIRIS/GTC imaging with tunable narrowband filters.

Keywords

supernovae: individual: SN 2008DSN 2007uySN 1999ehgalaxies: abundancestechniques: high angular resolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 169 - 170
Copyright
Copyright © International Astronomical Union 2015 

References

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