Kinematics and photometry as complementary tools in the study of barred galaxies

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dc.creatorBeltran, Juan Carlos Vega
dc.creatorErwin, Peter
dc.creatorBeckman, John
dc.creatorPizzella, Alessandro
dc.creatorCorsini, Enrico Maria
dc.creatorBertola, Francesco
dc.creatorZeilinger, Werner W.
dc.date2000-10-30
dc.date.accessioned2026-07-07T01:56:16Z
dc.date.available2026-07-07T01:56:16Z
dc.descriptionRecent advances in observational techniques and theoretical modelling of galaxy kinematics allow us to use more than just optical morphology to discern the structure and dynamics of galaxies. Here, we show for three barred galaxies (UGC 10205, NGC 6221 and NGC4340) that both kinematics and photometry are necessary to fully understand the properties of these galaxies. Kinematic and spectrophotometric data enable us to detect structures such as bars and gas shocks that are not directly visible in the images; conversely, imaging can be crucial for understanding the kinematic and dynamical behavior of a galaxy.
dc.description2 pages, 2 figures, to appear in the proceedings of "Galaxy Disks and Disk Galaxies," eds. J. G. Funes & E. M. Corsini (ASP Conference Series). Uses newpasp.sty (included)
dc.identifierhttps://arxiv.org/abs/astro-ph/0010593
dc.identifierhttp://arxiv.org/abs/astro-ph/0010593
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1935
dc.subjectAstrophysics
dc.titleKinematics and photometry as complementary tools in the study of barred galaxies
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