activity
20002012
most citedWarm Molecular Gas in Dwarf Starburst Galaxies: CO(3-2) Observations

88 citations · 340 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2012★ 15 cited

[S IV] in the NGC 5253 Supernebula: Ionized Gas Kinematics at High Resolution

Sara C. Beck, John H. Lacy, Jean L. Turner +3

The nearby dwarf starburst galaxy NGC 5253 hosts a deeply embedded radio-infrared supernebula excited by thousands of O stars. We have observed this source in the 10.5μm line of S+…

astro-ph2007★ 49 cited

CO(1-0), CO(2-1) and Neutral Gas in NGC 6946: Molecular Gas in a Late-Type, Gas Rich, Spiral Galaxy

Lucian Crosthwaite, Jean Turner

We present "On The Fly" maps of the CO(1-0) and CO(2-1) emission covering a 10' X 10' region of the NGC 6946. Using our CO maps and archival VLA HI observations we create a total g…

astro-ph2006★ 20 cited

Brackett Lines from the Super Star Cluster Nebulae in He 2-10

Alaina L. Henry, Jean L. Turner, Sara C. Beck +3

We present high spectral resolution (v~12-16 km/s) Brackett line spectroscopy of the blue compact dwarf galaxy Henize 2-10 made with NIRSPEC on the Keck Telescope. The spatial reso…

astro-ph2006★ 38 cited

Subarcsecond-Resolution Radio Maps of Nearby Spiral Galaxies

Chao-Wei Tsai, Jean L. Turner, Sara C. Beck +4

We report subarcsecond-resolution VLA imaging of four nearby spiral galaxies: IC 342, Maffei II, NGC 2903, and NGC 6946. In each galaxy, compact radio continuum sources are identif…

astro-ph2006

High Resolution Radio Maps of Four Nearby Spiral Galaxies

Chao-Wei Tsai, Jean L. Turner, Sara C. Beck +4

We report subarcsecond-resolution VLA imaging of the centers of four nearby spiral galaxies: IC 342, Maffei II, NGC 2903, and NGC 6946. In each galaxy, 7 - 12 compact radio continu…

astro-ph2003★ 62 cited

An extragalactic supernebula confined by gravity

J. L. Turner, S. C. Beck, L. P. Crosthwaite +3

Little is known about the origins of the giant star clusters known as globular clusters. How can hundreds of thousands of stars form simultaneously in a volume only a few light yea…