activity
19982004
collaborators
Showing astro-phShow all

5 papers · 1 filter

astro-ph2004

Probing Kolmogorov turbulence beyond the Magellanic Clouds: The Power of Southern Hemisphere's largest optical telescope (11m), SALT

D. L. Block, B. G. Elmegreen, D. M. Elmegreen +1

The Hubble classification scheme of galaxies is based on blue-light appearance. Atlases reveal the rich variety of responses of the Population I component (`the mask') of gas and d…

astro-ph2003

Penetration at high-z of the Greenberg "yellow stuff": Eyes to the Future with NGST

David L. Block, Ivanio Puerari, Marianne Takamiya +1

Quantitative morphological dust-penetrated templates for galaxies in our Local Universe may also serve as excellent templates for galaxies at high-z, because of partial/total decou…

astro-ph2001

The Duality of Spiral Structure, and a Quantitative Dust Penetrated Morphological Tuning Fork at Low and High Redshift

D. L. Block, I. Puerari, R. J. Buta +3

In the near-infrared, the morphology of older star-dominated disks indicates a simple classification scheme (1) H where is the dominant harmonic, (2) a pitch angle (derived…

astro-ph2000

The detection of spiral arm modulation in the stellar disk of an optically flocculent and an optically grand design galaxy

Ivanio Puerari, David L. Block, Bruce G. Elmegreen +2

Two dimensional Fourier spectra of near-infrared images of galaxies provide a powerful diagnostic tool for the detection of spiral arm modulation in stellar disks. Spiral arm modul…

astro-ph1998

Toward a dust penetrated classification of the evolved stellar Population II disks of galaxies

David L. Block, Ivanio Puerari

(abridged): To derive a coherent physical framework for the excitation of spiral structure in galaxies, one must consider the co-existence of two different dynamical components: a…