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arxiv: 0802.0610 · v1 · submitted 2008-02-05 · 🌌 astro-ph

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The pseudobulge of NGC 1292

L. Morelli (1) , E. Pompei (2) , A. Pizzella (1) , J. M\'endez-Abreu (1) , (3) , E. M. Corsini (1) , L. Coccato (4) , R. P. Saglia (4)
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M. Sarzi (5) F. Bertola (1) ((1) Dipartimento di Astronomia Universit\`a di Padova (2) European Southern Observatory (3) INAF-Osservatorio Astronomico di Padova (4) Max-Planck Institut f\"ur extraterrestrische Physik (6) Centre for Astrophysics Research University of Hertfordshire)
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classification 🌌 astro-ph
keywords pseudobulgepropertiesbuildupconsistentevolutionhostskinematicphotometric
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The photometric and kinematic properties of Sb NGC 1292 suggest it hosts a pseudobulge. The properties of the stellar population of such a pseudobulge are consistent with a slow buildup within a scenario of secular evolution.

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