The pseudobulge of NGC 1292

Simple item page
dc.creatorMorelli, L.
dc.creatorPompei, E.
dc.creatorPizzella, A.
dc.creatorMéndez-Abreu, J.
dc.creatorCorsini, E. M.
dc.creatorCoccato, L.
dc.creatorSaglia, R. P.
dc.creatorSarzi, M.
dc.creatorBertola, F.
dc.date2008-02-05
dc.date.accessioned2026-07-07T09:18:49Z
dc.date.available2026-07-07T09:18:49Z
dc.descriptionThe 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.
dc.description2 pages, 1 figure to appear in the proceedings of "Formation and Evolution of Galaxy Disks", Rome, October 2007, Eds. J. Funes and E. M. Corsini
dc.identifierhttps://arxiv.org/abs/0802.0610
dc.identifierhttp://arxiv.org/abs/0802.0610
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/154162
dc.subjectAstrophysics
dc.titleThe pseudobulge of NGC 1292
dc.typetext

Files

Collections

arXiv