activity
19972003
collaborators

7 papers

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-ph2002

A Fabry-Perot Study of the Scd I galaxy NGC 5457

Ivanio Puerari, Margarita Valdez-Gutierrez, Margarita Rosado

We have analyzed Halpha Fabry-Perot interferograms of NGC 5457 (M101) in order to calculate the rotation curve. We have also isolated a sample of 263 HII regions and we determined…

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 mass distribution of an optically flocculent galaxy

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

Spiral arm modulation in NGC 4062 (an optical flocculent) is detected for the first time; the Fourier spectra of NGC 4062 and NGC 5248 (a classic grand design in optical images) ar…

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…