The Toomre Sequence Revisited with HST/NICMOS: Nuclear Brightness Profiles and Colors of Interacting and Merging Galaxies

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dc.creatorRossa, Joern
dc.creatorLaine, Seppo
dc.creatorvan der Marel, Roeland P.
dc.creatorMihos, J. Christopher
dc.creatorHibbard, John E.
dc.creatorBoeker, Torsten
dc.creatorZabludoff, Ann I.
dc.date2007-08-20
dc.date.accessioned2026-07-07T11:18:43Z
dc.date.available2026-07-07T11:18:43Z
dc.descriptionWe discuss the near-infrared properties of the nuclei in the 11 merging galaxies of the Toomre sequence, based on high spatial resolution J, H, and K imaging data using NICMOS onboard the Hubble Space Telescope (HST). The observations are less affected by dust extinction than our previous HST/WFPC2 observations and offer higher spatial resolution than existing ground-based near-IR data. We see a marginal trend for the nuclei to become bluer with advancing merger stage, which we attribute to a dispersal of dust at late times in the merging process. Our data also indicate a statistically significant trend for the nuclei in the sequence to become more luminous, within an aperture of fixed physical size and after correcting for dust extinction, with advancing merger stage. We derive K-band surface brightness profiles for those nuclei for which the morphology allows a meaningful isophotal analysis, and fit the profiles with a ``Nuker law'' for comparison with other samples of galaxies observed with HST. The majority of the nuclei have steep profiles that can be characterized as power-law type. In general, the Toomre sequence galaxies tend to have steeper profiles and higher central luminosity surface densities than E/S0's. We derive V-K color profiles for the nuclei to further address this possibility, but find that the large amounts of dust extinction complicate their interpretation. Overall, our results are consistent with the generic predictions of N-body simulations of spiral galaxy mergers. If left to evolve and fade for several Gyrs, it is possible that the properties of the Toomre sequence nuclei would resemble theproperties of the nuclei of normal E/S0 galaxies. Our results therefore support the view that mergers of spiral galaxies can lead to the formation of early-type galaxies (Abridged).
dc.description46 pages, 25 figures, accepted for publication in AJ, article with full resolution images is available at http://www.stsci.edu/~marel/psgzdir/toomrenir.ps.gz
dc.identifierhttps://arxiv.org/abs/0708.2645
dc.identifierhttp://arxiv.org/abs/0708.2645
dc.identifierAstron.J.134:2124-2147,2007
dc.identifierdoi:10.1086/522782
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193440
dc.subjectAstrophysics
dc.titleThe Toomre Sequence Revisited with HST/NICMOS: Nuclear Brightness Profiles and Colors of Interacting and Merging Galaxies
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