activity
19972025
most citedInterstellar Turbulence I: Observations and Processes

1.2k citations · 20.6k across the 307 of their papers we have counts for

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Showing 2010Show all

12 papers · 1 filter

astro-ph.CO2010★ 52 cited

The thick disk in the galaxy NGC 4244 from S4G imaging

Sébastien Comerón, Johan H. Knapen, Kartik Sheth +16

If thick disks are ubiquitous and a natural product of disk galaxy formation and/or evolution processes, all undisturbed galaxies which have evolved during a significant fraction o…

astro-ph.CO2010

A New Method for Measuring the Upper End of the IMF

Daniela Calzetti, Rupali Chandar, Janice C. Lee +3

A method is presented here for investigating variations in the upper end of the stellar Initial Mass Function (IMF) by probing the production rate of ionizing photons in unresolved…

astro-ph.CO2010★ 521 cited

The Spitzer Survey of Stellar Structure in Galaxies (S^4G)

Kartik Sheth, Michael Regan, Joannah L. Hinz +35

The Spitzer Survey of Stellar Structure in Galaxies S^4G is an Exploration Science Legacy Program approved for the Spitzer post-cryogenic mission. It is a volume-, magnitude-, and…

astro-ph.CO2010★ 41 cited

Tadpole Galaxies in the Hubble Ultra Deep Field

Bruce G. Elmegreen, Debra Meloy Elmegreen

Tadpole galaxies have a head-tail shape with a large clump of star formation at the head and a diffuse tail or streak of stars off to one side. We measured the head and tail masses…

astro-ph.GA2010★ 21 cited

Mass Functions in Fractal Clouds: The Role of Cloud Structure in the Stellar Initial Mass Function

Mohsen Shadmehri, Bruce G. Elmegreen

The possibility that the stellar initial mass function (IMF) arises mostly from cloud structure is investigated with fractal Brownian motion (fBm) clouds that have power-law power…

astro-ph.CO2010★ 1 cited

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…