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Planetary nebulae as tracers of the kinematic structure of the starburst galaxy IC 10

Published online by Cambridge University Press:  30 August 2012

Denise R. Gonçalves
Affiliation:
UFRJ - Observatório do Valongo, Ladeira Pedro Antonio 43, 20080-090 Rio de Janeiro, Brazil. Email: [email protected] Department of Physics and Astronomy, University College London, Gower Street, WC1E 6BT London, UK
Ana M. Teodorescu
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, HI 96822 Honolulu, USA. Email: [email protected]; [email protected]
Alan Alves-Brito
Affiliation:
PUC, Departamento de Astronomia y Astrofísica, Av. Vicuña Mackenna 4860, 782-0436 Santiago, Chile. Email: [email protected]
Roberto H. Méndez
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, HI 96822 Honolulu, USA. Email: [email protected]; [email protected]
Laura Magrini
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy. Email: [email protected]
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Abstract

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The Local Group dwarf irregular galaxy IC 10 is the nearest starburst galaxy (at 725 kpc) and presents extended and complex HI kinematics. It is believed that IC 10 is still experiencing an intense and very recent burst of star formation, likely triggered by infalling gas from an extended envelope which is counter-rotating with respect to the galaxy proper rotation. In this contribution we summarize our preliminary results (Gonçalves et al. 2011, in prep.) obtained by performing a kinematic analysis of the PN population of IC 10. Our aim is to explore the kinematic connection of its intermediate to old stellar populations with that obtained from HI observations. Some PNe were found at large galactocentric distances and could therefore represent a trace of past tidal interactions.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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