papers

Publications (13)

astro-ph2007

Keck spectroscopy and Spitzer Space Telescope analysis of the outer disk of the Triangulum Spiral Galaxy M33

David L. Block, Francoise Combes, Ivanio Puerari +11

In an earlier study of the spiral galaxy M33, we photometrically identified arcs or outer spiral arms of intermediate age (0.6 Gyr - 2 Gyr) carbon stars precisely at the commenceme…

astro-ph.CO2010

The Large Magellanic Cloud: A power spectral analysis of Spitzer images

Ivanio Puerari, David L. Block, Bruce G. Elmegreen +1

We present a power spectral analysis of Spitzer images of the Large Magellanic Cloud. The power spectra of the FIR emission show two different power laws. At larger scales (kpc) th…

astro-ph2002

Gravitational torques in spiral galaxies: gas accretion as a driving mechanism of galactic evolution

David L. Block, Frederic Bournaud, Francoise Combes +2

The distribution of gravitational torques and bar strengths in the local Universe is derived from a detailed study of 163 galaxies observed in the near-infrared. The results are co…

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-ph2004

Dust penetrated arm classes: insight from rising and falling rotation curves

Marc S. Seigar, David L. Block, Ivanio Puerari

We present near-infrared K-band images of 15 galaxies. We have performed a Fourier analysis on the spiral structure of these galaxies in order to determine their pitch angles and d…

astro-ph2007

Variation of Galactic Bar Length with Amplitude and Density as Evidence for Bar Growth over a Hubble Time

Bruce G. Elmegreen, Debra Meloy Elmegreen, Johan H. Knapen +3

K_s-band images of 20 barred galaxies show an increase in the peak amplitude of the normalized m=2 Fourier component with the R_25-normalized radius at this peak. This implies that…