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20002023
most citedRe-examining Larson's Scaling Relationships in Galactic Molecular Clouds

659 citations · 7.4k across the 73 of their papers we have counts for

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Showing 2008Show all

6 papers · 1 filter

astro-ph2008

Spectra of Nearby Galaxies Measured with a New Very Broadband Receiver

Gopal Narayanan, Ronald L. Snell, Neal R. Erickson +4

Three-millimeter-wavelength spectra of a number of nearby galaxies have been obtained at the Five College Radio Astronomy Observatory (FCRAO) using a new, very broadband receiver.…

astro-ph2008★ 82 cited

The Molecular Properties of Galactic HII Regions

L. D. Anderson, T. M. Bania, J. M. Jackson +5

We derive the molecular properties for a sample of 301 Galactic HII regions including 123 ultra compact (UC), 105 compact, and 73 diffuse nebulae. We analyze all sources within the…

astro-ph2008★ 659 cited

Re-examining Larson's Scaling Relationships in Galactic Molecular Clouds

Mark Heyer, Coleman Krawczyk, Julia Duval +1

The properties of Galactic molecular clouds tabulated by Solomon etal (1987) (SRBY) are re-examined using the Boston University-FCRAO Galactic Ring Survey of 13CO J=1-0 emission. T…

astro-ph2008★ 126 cited

The Five College Radio Astronomy Observatory CO Mapping Survey of the Taurus Molecular Cloud

Gopal Narayanan, Mark H. Heyer, Christopher Brunt +3

The FCRAO Survey of the Taurus Molecular Cloud observed the 12CO and 13CO J=1-0 emission from 98 square degrees of this important, nearby star forming region. This set of data with…

astro-ph2008★ 486 cited

Large-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping

Paul F. Goldsmith, Mark Heyer, Gopal Narayanan +3

We report the results of a 100 square degree survey of the Taurus Molecular Cloud region in the J = 1-0 transition of 12CO and 13CO. The image of the cloud in each velocity channel…

astro-ph2008★ 140 cited

Magnetically Aligned Velocity Anisotropy in the Taurus Molecular Cloud

Mark Heyer, Hao Gong, Eve Ostriker +1

Velocity anisotropy induced by MHD turbulence is investigated using computational simulations and molecular line observations of the Taurus molecular cloud. A new analysis method i…