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19982014
most citedISM properties in hydrodynamic galaxy simulations: Turbulence cascades, cloud formation, role of gravity and feedback

225 citations · 767 across the 18 of their papers we have counts for

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12 papers · 1 filter

astro-ph2007★ 57 cited

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…

astro-ph2007★ 14 cited

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-ph2006★ 72 cited

Fourier Dissection of Early-Type Galaxy Bars

R. Buta, E. Laurikainen, H. Salo +2

This paper reports on a near-infrared survey of early-type galaxies designed to provide information on bar strengths, bulges, disks, and bar parameters in a statistically well-defi…

astro-ph2006★ 105 cited

The Near-infrared S0 Survey III: Morphology of 15 Southern Early-type Disk Galaxies

E. Laurikainen, H. Salo, R. Buta +3

Structural analysis has been performed for a sample of 15 Southern early-type disk galaxies, mainly S0s, using high resolution -band images. The galaxies are mostly barred and…

astro-ph2006★ 35 cited

Pseudobulges in the Disk Galaxies NGC 7690 and NGC 4593

John Kormendy, Mark E. Cornell, David L. Block +2

We present Ks-band surface photometry of NGC 7690 (Hubble type Sab) and NGC 4593 (SBb). We find that, in both galaxies, a major part of the "bulge" is as flat as the disk and has a…

astro-ph2004★ 25 cited

Very Luminous Carbon Stars in the Outer Disk of the Triangulum Spiral Galaxy

D. L. Block, K. C. Freeman, T. H. Jarrett +4

Stars with masses in the range from about 1.3 to 3.5 Mo pass through an evolutionary stage where they become carbon stars. In this stage, which lasts a few Myr, these stars are ext…